Refine
Year of publication
Document Type
- Doctoral Thesis (44)
- Article (1)
Has Fulltext
- yes (45)
Is part of the Bibliography
- no (45)
Keywords
- Plasma (45) (remove)
Institute
- Institut für Physik (25)
- Institut für Hygiene und Umweltmedizin (6)
- Institut für Pharmazie (4)
- Klinik und Poliklinik für Chirurgie Abt. für Viszeral-, Thorax- und Gefäßchirurgie (2)
- Abteilung für Mikrobiologie und Molekularbiologie (1)
- Institut für Immunologie u. Transfusionsmedizin - Abteilung Transfusionsmedizin (1)
- Institut für Klinische Chemie und Laboratoriumsmedizin (1)
- Interfakultäres Institut für Genetik und Funktionelle Genomforschung (MNF) (1)
- Klinik und Poliklinik für Chirurgie Abt. für Unfall- und Wiederherstellungschirurgie (1)
- Klinik und Poliklinik für Hals-, Nasen-, Ohrenkrankheiten, Kopf- und Halschirurgie (1)
- Klinik und Poliklinik für Urologie (1)
- Poliklinik für Kieferorthopädie, Präventive Zahnmedizin und Kinderzahnheilkunde (1)
Publisher
- S. Karger AG (1)
Recent experimental campaigns in the Wendelstein 7-X stellarator, a
plasma-confining device designed to investigate the Magnetic Confinement Fusion
(MCF) approach to generating electrical power, have shown that the injection of
fuelling pellets had an unexpected and considerable impact on the performance of
the plasma. Rather than simply refuelling the device and `diluting' the plasma
energy, pellet injection is followed by a significant increase in the ratio of
the ion temperature to the electron temperature. It has been suggested that this
is not merely due to the improved confinement following the reduction of
turbulent transport after the pellet material has homogenised with the bulk
plasma, but also due to a direct transfer of energy from electrons to ions. The
proposed mechanism for this energy transfer is the ambipolar expansion of the
pellet plasmoid, the localised plasma structure produced by the
ionisation of ablated pellet material, along magnetic field lines.
Early work on pellet plasmoid expansion predicted that half the heating power
deposited in plasmoid electrons by collisions with hot ambient electrons is
transferred to plasmoid ions in the form of flow velocity as the plasmoid
expands. The complicated nature of the system of the pellet plasmoid embedded in
the ambient plasma, particularly the behaviour of electrons, which experience
many collisional and collisionless phenomena on multiple disparate timescales,
means that early models of the expansion were not wholly self-consistent, but
rather made use of strong approximations that apply in some regions of the
plasmoid but not in others. For example, only electrons and ions associated with
the plasmoid were rigorously treated, meaning that the framework was one of
`expansion into vacuum'. Combined with the assumption of Maxwellian electrons,
this led to an electric potential that was unbounded at infinity. Naturally, the
validity of the conclusions of such a model are called into question because the
approximations lose their validity far from the plasmoid and as time advances,
yet predictions about the final state of the plasma are desired. A deeper
investigation is required: careful consideration of the phenomena in question
and the timescales (and lengthscales) on which they act must be made in order to
rigorously construct a model that is valid throughout the entire expansion.
The first two papers presented in this thesis iterate on the model established
in the paper that first predicted the electron-to-ion energy transfer; their aim
was to find out how the character of the expansion changes with a more
sophisticated and accurate description of various phenomena, while remaining
within the existing framework of expansion into vacuum. Ultimately, we find that
the qualitative character is unchanged, and that approximately half the heating
power deposited in plasmoid electrons is transferred to ions.
Two other papers in this thesis address the limitations of the original model.
This is achieved by properly considering the electron kinetic problem in a
plasmoid. One paper considers the electron kinetic problem when electrons are
highly isotropised. In this case the kinetic equation can be integrated to
remove all but two independent variables, which is the maximum possible
reduction considering it is a time-dependent problem. The full nonlinear
integro-differential Landau self-collision operator is integrated exactly and
few approximations are made, leading to a rather general kinetic equation.
However, for fuelling pellets some anisotropy in the electron distribution is
expected. Another paper considers the electron kinetic problem (and the entire
plasmoid expansion) allowing for electron anisotropy. Careful consideration of
the ordering of timescales of electron phenomena in a pellet plasmoid leads to a
steady-state kinetic problem that we call collisional quasi-equilibrium (QE). QE
appears in many ways similar to the collisional steady-state characterising a
true thermal equilibrium. It was found that the time-dependent kinetic problem
of the earlier paper, with isotropic electrons, produces the QE distribution
function, corroborating the existence of the QE state. We then take moments of
the electron kinetic equation that is valid on the expansion timescale, assuming
that the electron distribution is that given as the solution to the QE kinetic
problem. This is completely analogous to what is done to obtain the Braginskii
equations or any Chapman-Enskog theory. The result is a set of equations for the
long-term evolution of the macroscopic quantities that describe the distribution
function existing in a quasi-steady-state at each point in time. It is from this
point that one may feasibly describe the plasmoid expansion with an accurate
picture of the electron kinetics and finally obtain the electron-to-ion energy
transfer so desired in a rigorous model of the expansion.
From a broader point of view, the two frameworks provided by these rigorous
investigations of the electron kinetic problem serve as a basis for the future
study of plasmoids. Such a `first-principles' approach to plasmoid dynamics is
novel and interesting in its own right, but it will be demonstrated that such an
approach is essential for pellet plasmoids owing to the fact that they are
poorly described by the `standard tools' of plasma physics.
Using the QE framework it was found that, once more, about half the heating
power experienced by plasmoid electrons is transferred to plasmoid ions. The
incredible robustness of the prediction of such an energy transfer is, in the
author's opinion, the result of the self-similar nature of the expansion found
as a solution to the original model. As a rule, the profiles of self-similar
solutions tend to be attractors for the `real', more complicated, system, and
the qualitative predictions involving no parameters, of which the
electron-to-ion energy transfer is one, tend to be very sturdy.
Aside from fuelling pellets, composed of hydrogen or deuterium, one paper in
this thesis investigates the physics of high-Z pellets that are designed to
terminate the plasma safely in the event of a `disruption', where much of the
magnetic field energy is channelled into a runaway electron beam with
potentially disastrous consequences if the beam encounters a plasma-facing
component. The paper draws on the work carried out in the paper concerning the
kinetic problem of isotropised electrons in a plasmoid.
This thesis is `cumulative'; the vast majority of the work carried out is
described within a set of Papers, labelled A-E, placed at the back of the text.
There is a preceding `wrapper text' (given in numbered Sections) tasked with
introducing the reader to the topic, guiding the reader through the papers, and
expounding some of their main results. Some amount of material not present in
the papers is also provided in the wrapper text. Naturally, the wrapper text
mainly focusses on the results of the papers which are under my first
authorship. In the course of publishing papers over an extended period of time
the nomenclature is bound to vary. Although it is mostly consistent between the
papers, a few difference do arise, and the section `Common symbols and
subscripts' is provided in the frontmatter to alleviate confusion. Particular
care should be taken with the symbols x and z; both can refer to the
coordinate parallel to the magnetic field line, but in papers where z is used
for this purpose x tends to have another definition. In the wrapper text the
choice of symbols is generally chosen to reflect those in the corresponding
paper.
Einfluss der Plasmabehandlung auf das transepidermale Penetrationsverhalten von Arzneistoffen
(2021)
Zusammenfassung und Ausblick
Die Forschungshypothese, dass eine Plasmabehandlung der Haut mit kaltem
Atmosphärendruckplasma zu einer lokalen Änderung der physikochemischen Eigenschaften des
Stratum corneum und dessen Struktur und (Barriere-)Funktion führt, konnte bestätigt werden.
Im Rahmen der vorliegenden Arbeit wurden morphologisch sichtbare Hautveränderungen, die
Penetrationseigenschaften verschiedener Substanzen vor und nach Plasmabehandlung sowie
Veränderungen der Lipidzusammensetzung des Stratum corneum auf molekularer Ebene analysiert.
Der wesentliche Erkenntnisgewinn der Arbeit besteht im qualitativen und quantitativen Nachweis der
gefahrlosen durch kaltes Atmosphärendruckplasma vermittelten Penetrationssteigerung von
Substanzen in die Haut mit speziellem Fokus auf das Stratum corneum.
Die Plasmabehandlung der Haut mit einem Plasmajet lockert abhängig von der
Plasmabehandlungszeit das aus Corneozyten und einer interzellulären Lipidmatrix bestehende
Stratum corneum auf. Die aufgelockerte Struktur des Stratum corneum ermöglicht eine beschleunigte
Penetration verschiedener, nach Plasmabehandlung applizierter Substanzen durch die Haut (Kapitel
4.2.). Die Penetrationssteigerung variiert dabei abhängig von den Stoffeigenschaften der
penetrierenden Substanz (zum Beispiel Molekülgröße und Lipophilie).
Die morphologische Auflockerung des Stratum corneum spiegelt sich im nach der Plasmabehandlung
veränderten Ceramid-Profil wieder. Die veränderten Barriereeigenschaften in den obersten Schichten
des Stratum corneum nach einer einminütigen Plasmabehandlung lassen sich über die Interaktion von
plasma-produzierten reaktiven Spezies mit Lipiden der Haut (insbesondere Triacylglycerolen) und
die dadurch vermittelte Bildung von Triacylglycerol-Oxidationsprodukten erklären (Kapitel 4.4.).
Eine Plasmabehandlung hat im Bereich der in der Dermatologie für den kINPen MED empfohlenen
Anwendungsdauer von 15 s/cm² bis 1 min/cm² keine negativen Auswirkungen auf die Haut (keine
gesteigerte Anzahl an Apoptosen im Stratum basale, Möglichkeit der Regeneration des
aufgelockerten Stratum corneum von basal, (Kapitel 4.3.)). Längere Behandlungszeiten von 2
min/cm² bis 5 min/cm² können jedoch zu Apoptosen in für die Zellregeneration bedeutenden
Schichten führen.
Im Gegensatz zu anderen Methoden zur transdermalen Penetrationssteigerung besteht bei der Plasma-
vermittelten Penetrationssteigerung auf Grund der antibakteriellen Plasmaeigenschaften und der
Penetrationsbeschleunigung von ausschließlich kleinen Stoffen (Größe unter 689 nm) ein geringeres
Risiko der Infektion der behandelten Hautbereiche durch die Einwanderung von Bakterien und
Pilzen. Die Plasmabehandlung stellt demnach eine zukunftsträchtige Möglichkeit zur gefahrlosen
Penetrationssteigerung von Arzneistoffen durch die Hautbarriere dar.
Da die in dieser Arbeit gewonnenen Daten in vitro mit Hilfe eines Schweineohrmodells ermittelt
wurden, ermöglichen sie einen ersten Einblick in die Reaktion der gesunden menschlichen Haut auf
die Plasmabehandlung, lassen sich jedoch nicht eins zu eins auf die in vivo-Situation am menschlichen
Körper übertragen. Zudem sollte bei der Plasmabehandlung in vivo beachtet werden, dass es am
menschlichen Körper große intra- und interindividuelle Unterschiede in der Beschaffenheit der
Hautbarriere gibt, welche zu unterschiedlich starken Effekten der Plasmabehandlung führen könnten.
Ein Vergleich der Penetrationseigenschaften weiterer Stoffe mit unterschiedlichen hydro- und
lipophilen Stoffeigenschaften sowie unterschiedlichen Molekülgrößen vor und nach
Plasmabehandlung wäre für weitere Forschungsarbeiten empfehlenswert. Auf diese Weise könnte
erforscht werden, auf welche Substanzen die Plasmabehandlung der Haut den größten Einfluss hat
und es wären weitere Rückschlüsse auf die Form der aufgelockerten Bindungen, sowie auf eine
eventuelle Interaktion modifizierter Stratum corneum-Bestandteile mit der penetrierenden Substanz
möglich. Gleichzeitig könnten die Versuche mit längeren Penetrationszeiten wiederholt werden, um
zu überprüfen, ob tatsächlich eine Rechtsverschiebung des Peaks der Konzentration der penetrierten
Substanzen (siehe Kapitel 3.4. und Kapitel 3.5.) in tiefere Hautbereiche stattfindet.
Ein direkter Vergleich penetrationssteigernder Methoden (beispielsweise Mikronadeln und
Plasmajet) wäre interessant, um die verschiedenen Systeme auch quantitativ vergleichen zu können
und zu analysieren, ob die Vorteile der plasmavermittelten Penetrationssteigerung gegenüber der
Mikronadelmethode durch die Menge an penetrierter Substanz ausgeglichen werden können.
Neben den Lipiden könnte auch die Modifikation weiterer Stratum-corneum-Bestandteile ursächlich
für die veränderten Barriereeigenschaften der Haut nach Plasmabehandlung sein. Interessant wäre
deshalb auch die Untersuchung der Stratum-corneum-Peptide und -Proteine vor und nach
Plasmabehandlung.
Um die Reaktion der Haut in vivo auf die Plasmabehandlung besser vorhersagen zu können und damit
die im Rahmen dieser Arbeit erlangten Erkenntnisse in die klinische Praxis übertragen zu können,
sind weitere Studien nötig. Diese könnten die in vitro-Experimente am Schweineohr beispielsweise
auf ein in vivo-Mäusehautmodell übertragen. An einem frischen Mäusehautmodell wäre auch die
Untersuchung längerer Penetrationszeiten sowie die Geschwindigkeit der Hautregeneration und dem
damit Verbundenen Wiederaufbau der Hautbarriere nach Plasmabehandlung möglich.
Nach einer Verifizierung der Ergebnisse in vivo könnten die im Rahmen dieses Projekts gewonnenen
Erkenntnisse in Zukunft auf den klinischen Alltag übertragen werden. Für Langzeittherapien bei
speziellen Patientengruppen mit Problemen bei der oralen Medikamentenaufnahme (beispielsweise
in Form von Resorptionsstörungen im Magen-Darm-Trakt) oder bei einem starken First-Pass-Effekt
des Medikaments in der Leber ist die transdermale Medikamentenapplikation eine
Ausweichmöglichkeit, welche durch eine vorherige Plasmabehandlung der Haut noch verbessert
werden würde.
Im Rahmen des bereits etablierten medizinischen Anwendungsfelds von kaltem
Atmosphärendruckplasma bei der Behandlung chronischer Wunden könnte eine Plasmabehandlung
der Wundränder und angrenzender gesunder Hautbereiche die Penetration von nach der Behandlung
applizierten wundheilungsfördernden Cremes und Gels im betroffenen Gebiet beschleunigen und so
die Heilungsaussichten noch weiter verbessern.
Objectives:
This study investigates the effectiveness of the Cold AP on the alteration of the enamel surface
without using acid etchant by using Conventional photo-activated resin bond to bond the
orthodontic brackets.
Materials and Methods:
One hundred and twenty-five Enamel specimens are prepared from disinfected bovine
mandibular incisors are divided into five groups. Group I: brackets are attached on the enamel
surface with the standard adhesive technique (etch + primer +bond). Group II: the brackets are
attached with the Standard Orthodontic adhesive technique without etching. Group III: the
enamel surface is conditioned with pure Argon Cold atmospheric plasma before the application
of the primer without using an acid etchant. Group IV: the enamel surface is conditioned with
the admixture of Argon Cold atmospheric plasma with 0.5 % Oxygen before the application of
the primer without using acid etchant Group V: after the application of Argon Cold atmospheric
plasma with 0.5 % Oxygen the surface is rewetted by deionized water before the application
of the primer and adhesive. After that, the samples are exposed to thermal cycling. The shear
bond strength of the samples is tested by the universal testing machine which measured the
maximum force at which the brackets are deboned from the tooth surface at a speed of
1mm/minute is measured.
Results:
Significant intergroup differences were found. Group V showed the highest shear bond
strength followed by Group I, VI, III, II respectively. There isn’t a statistical difference in the
values of The Shear bond strength values between Group III and IV.
Conclusions:
this study implies that Cold Atmospheric Plasma is a safe method to change the chemical
surface characteristics of the enamel surface.in addition to the significant importance of plasma
treatment followed by water rewetting, which could enhance adhesion between the orthodontic
attachments and the enamel layer
Untersuchung zur Wirkung von kaltem Atmosphärendruckplasma über die Oxidation von Thiolgruppen
(2022)
Redox signaling-Prozesse innerhalb und zwischen Zellen spielen eine Rolle in
verschiedenen physiologischen und pathologischen Prozessen, wobei zelluläre
Thiolgruppen als wichtige Signalübermittler identifiziert wurden. Durch Behandlung der
Aminosäure Cystein mit kaltem Atmosphärendruckplasma werden solche
Thiolgruppen oxidiert und verschiedene Verbindungen erzeugt. Diese Arbeit sollte
klären, ob so die Erzeugung von stabilen reaktiven Spezies möglich ist, die einen
biologischen Effekt haben. Dazu wurden Pufferlösungen, die Cystein enthielten, mit
einem Argon-Plasmajet (kINPen 09) mit Sauerstoffzumischung behandelt und auf
kultivierte menschliche Keratinozyten der HaCaT-Zellinie übertragen. Zellproliferation,
Migrationsaktivität, Metabolismus, Viabilität und intrazellulärer Redoxzustand wurden
untersucht.
Plasmabehandelte Flüssigkeiten mit Cysteinkonzentrationen von 2 mmol/l zeigten
keinen Einfluss auf das Zellverhalten im Vergleich zu behandeltem Puffer ohne
Cystein. Erhöhte Cysteinkonzentrationen von 100 mmol/l verringerten bei langen
Plasmabehandlungszeiten von 5 min beziehungsweise 10 min die Proliferation,
Migration, Laktatsekretion und Viabilität. Für kürzere Behandlungszeiten von 1 min und
2,5 min wurden Hinweise auf eine erhöhte metabolische Aktivität gefunden. GSSGSpiegel
in den Zellen wurden stabilisiert und intrazelluläre ROS reduziert. Diese
Effekte könnten auf generierte bioaktive Substanzen wie oxidierte Disulfide
zurückzuführen sein, die längerfristig zu Energiemangel führen. Ein möglicher
Vermittler ist Cystein-S-sulfonat, welches als NMDA-Rezeptoragonist bekannt ist.
Zudem könnte auch die Aktivierung des XC-Antiporters mit Folgen für den
intrazellulären Redoxzustand zu den kurzfristigen Effekten beigetragen haben.
Durch plasmabehandelte Cysteinlösung konnten biologische Effekte, teilweise im
Sinne einer Hormesis, nachgewiesen werden. Die Ergebnisse zeigten eine
zytotoxische Wirkung nach langer Plasmabehandlung der Cysteinlösung, während für
kürzere Zeiten auch aktivierende Effekte deutlich wurden. Somit scheint die gezielte
Erzeugung stabiler reaktiver Spezies als neuer Ansatzpunkt der Plasmaanwendung
möglich.
Kinetic modeling and infrared spectroscopy of charge carriers across the plasma-wall interface
(2022)
In this thesis, charge transport at the plasma-wall interface is investigated theoretically, on a semiclassical, microscopic level. Based on the Boltzmann and Poisson equations a set of equations is derived and numerically solved to model charge carriers both within a semiconducting wall and a gaseous plasma in front of it. While the plasma is considered collision-free, within the solid, phonon collisions, as well as recombination processes between conduction band electrons and valence band holes are considered. This results, for the first time, in a self-consistent modeling of both the gaseous electron-ion plasma and the electron-hole plasma in the solid on the same footing. Utilizing specific approximations for different physical scenarios, numerical solutions are presented both for the floating and the electronically contacted (biased) interface. In the latter case, the current voltage characteristic is calculated and shown to heavily depend on the charge kinetics within the wall.
Furthermore, we present optical methods to measure the wall charge noninvasively. These utilize the influence of the deposited surplus charges on the optical reflection coefficient of the surface. By calculating the optical response of these charges, we show that the magnitude of the surface charge can be inferred from the change in the reflectivity of the surface caused by the presence of the plasma. While nonlocal effects are considered, it is shown analytically and numerically that these can be neglected at the scales of the considered physical systems.
Kaltes Atmosphärendruckplasma (CAP) hat in der Therapie an Bedeutung gewonnen und wird zurzeit in verschiedenen Bereichen der Medizin eingesetzt. CAP hat antiproliferative, antimikrobielle und zellstimulierende Wirkungen. Eine therapeutisch vielversprechende Einsatzmöglichkeit vom CAP ist die Behandlung maligner Tumoren. Weiterhin wird CAP klinisch in der Behandlung chronischer Wundheilungsstörungen der Haut eingesetzt.
In dieser Arbeit wurde die antiproliferative Wirkung von CAP auf zwei Haut-assoziierte Zelllinien (HaCaT und B16) untersucht. Anhand der CAP-Exposition und der Analyse der Wachstumskinetiken konnten wir bestätigen, dass die antiproliferative Wirkung von CAP von der Behandlungszeit abhängt. Ferner bestätigten die Ergebnisse, dass die antiproliferative Wirkung in der malignen Zelllinie B16 stärker ausgeprägt ist.
Weiterhin wurde die genotoxische Wirkung von CAP in einem 3D-Epidermismodell, dem epiCS® untersucht. Das Epidermismodell wurde 30s, 60s und 120s mit CAP behandelt (Plasmagerät kINPen MED). Zum Nachweis von DNA- Doppelstrangbrüchen und Apoptose wurden γ-H2AX und Caspase-3 herangezogen. Die fluoreszenzmikroskopische Analyse der Epidermis zeigte keinen höheren Anteil an γ-H2AX oder Capspase-3 positiven Zellen durch die CAP-Exposition. Lediglich waren γ-H2AX und Caspase-3 in beiden Behandlungsgruppen (Argon/CAP) nachweisbar. Ein direkter Zusammenhang zur CAP-Behandlung bzw. zur Behandlungszeit wurde jedoch nicht nachgewiesen.
Insgesamt kann man feststellen, dass die CAP-Exposition nicht zur vermehrten Apoptose in gesunden Epidermiszellen führt. Außerdem kann die CAP-Exposition gesunder Epidermis Zellen bis 120s ohne genotoxische oder zellschädigende Wirkung erfolgen.
In dieser Arbeit sollte die Möglichkeit der Anwendung von kaltem atmosphärischen Plasma (CAP) bei der Therapie von Plattenepithelkarzinomen des Kopf-Hals-Bereichs (HNSCC) evaluiert werden. Dazu wurden in vitro HNO97- und HNO41-Karzinomzellen mit Argon-CAP bzw. Helium-CAP durch den kINPen 09 bzw. einen Prototyp behandelt und einer Epithelzelllinie gegenübergestellt, um quellgasbedingte Unterschiede herauszuarbeiten. Durch die Verwendung von fetalem Kälberserum (FCS) und Panexin NTA (NTA) konnten zwei unterschiedliche Mediumzusätze verglichen werden.
In Wachstumskinetiken wurde eine Reduktion der Zellzahl von Karzinom- und Epithelzellen nach CAP-Behandlung erzielt. Daran schloss sich eine Proteomanalyse durch 2D-DIGE mit mas- senspektrometrischer Identifikation von in ihrer Menge veränderten Proteinen im Vergleich zu korrespondierenden Gaskontrollen an. Durch eine Hauptkomponentenanalyse (PCA) regu- lierter Proteine konnten die behandelten Proben in Cluster aufgeteilt werden. Die Auftrennung war in absteigender Effektgröße abhängig vom verwendeten Serum, Quellgas und der CAP-Behandlung. Mit Hilfe von Ingenuity Pathway Analysen (IPA) wurden Regulatorproteine und molekulare Funktionen identifiziert. So ließ sich die Regulation von p53, HSF1 und TGF-b und eine damit verbundene Beeinflussung der Stressantwort auf ungefaltete Proteine, der mitochondrialen Membranpermeabilität und der Apoptose nachweisen. Durch Darstellung der regulierten Proteine in Netzwerken konnte der Einfluss von CAP auf den MAPK-ERK-Pathway als zentraler Bestandteil der Wirkung identifiziert werden.
Nach Analyse der Proteinveränderungen wurde explizit eine mögliche Beeinflussung von Hit- zeschockprotein 27 (HSP27) und Glycerinaldehyd-3-phosphat Dehydrogenase (GAPDH) mittels Immunoblotassay untersucht. HSP27 dient u.a. der Reduktion von oxidativem Stress. GAPDH ist in Abhängigkeit vom Oxidationsstatus Bestandteil der Glykolyse oder an der Apoptose beteiligt. Es zeigte sich eine Reduktion der Proteinmenge von HSP27 durch CAP in Karzinomzellen, die unter Verwendung von NTA größer ausfiel als unter FCS. Die Proteinmenge von GAPDH änderte sich nicht, es ließ sich lediglich eine Modifikation des Proteins vermuten.
Die Ergebnisse dieser Arbeit zeigen, dass Karzinomzellen an oxidativen Stress nur bedingt anpassungsfähig sind und CAP somit eine geeignete Therapieoption darstellt. Die Effektivität des CAP wird dabei durch das Quellgas, die Behandlungsdauer sowie extra- und intrazelluläre Scavengersysteme beeinflusst.
Schilddrüsenhormone haben einen vielfältigen Einfluss auf den Stoffwechselmetabolismus. Die genauen molekularen Mechanismen, die mit Veränderungen der Schilddrüsenhormon-spiegel einhergehen, sind jedoch in vielen Bereichen noch unbekannt. Das Ziel der Arbeit bestand deshalb darin, auf Basis von Daten einer repräsentativen Stichprobe der Allgemein-bevölkerung die Zusammenhänge zwischen den Schilddrüsenhormonen und einem umfang-reichen Metabolitenpanel zu untersuchen, um so weitere Einblicke in die zugrunde-liegenden Ätiologien und Signal-wege zu erhalten.
Von 952 Teilnehmenden der SHIP-Trend-Studie wurden aus Plasma- und Urinproben in einem kombinierten Messverfahren (LC-MS sowie 1H-NMR) sowohl mit ungerichtetem als auch mit gerichtetem Ansatz das Metabolom quantifiziert. Um den Zusammenhang zwischen Thyroxin (fT4), Triiodthyronin (fT3) und Thyreotropin (TSH) mit den identifizierten Metaboliten zu untersuchen, wurden lineare Regressionsmodelle herangezogen. Bei Vorliegen eines signi-fikanten Interaktionseffekts zwischen fT4, fT3 bzw. TSH und dem Geschlecht wurden diese Analysen für Männer und Frauen getrennt durchgeführt. Eine Random-Forest-Analyse wurde angewendet, um die Relevanz phänotypischer Charakteristiken für die individuelle fT4-Konzentration vorherzusagen und die beobachteten Geschlechterunterschiede in den Asso-ziationen zu erklären.
Zwischen TSH und den Metaboliten im Plasma und Urin ließen sich keine signifikanten Assoziationen identifizieren. 106 von 613 Plasmametaboliten waren signifikant mit fT4 assoziiert. Assoziationen zwischen fT4 und den Urinmetaboliten ließen sich hingegen deutlich seltener beobachten (12 von 587). Die Mehrheit der mit fT4 assoziierten Plasmametabolite (n = 84) konnte den Klassen der Lipide und Lipidabkömmlingen zugeordnet werden. Die Analyse unterschiedlicher, mittels 1H-NMR-Spektroskopie quantifizierter Lipoproteinsub-fraktionen zeigte zudem in-verse Assoziationen zwischen der fT4-Konzentration und einer Reihe von großen sowie kleinen LDL- und HDL-Unterklassen auf. Dabei ließen sich auch einige geschlechtsspezifische Assoziationen beobachten. So konnten beispielsweise die Assoziationen zwischen fT4 und den HDL3-Subfraktionen nur bei Männern beobachtet werden. Assoziationen zwischen fT4 und verschiedenen mehrfach ungesättigten sowie gesättigten Fettsäuren waren hingegen nur bei Frauen sichtbar. Die identifizierten Geschlechterunterschiede in den Assoziationen lassen sich vermutlich bei Männern auf einen höheren Alkoholkonsum und bei Frauen auf Vorerkrankungen der Schilddrüse sowie den menopausalen Status zurückführen, denn die genannten phänotypischen Charakteristiken zeigten sich in den Random-Forest-Analysen als wichtige geschlechtsspezifische Faktoren für den individuellen fT4-Spiegel. Assoziationen zwischen fT3 und den Metaboliten im Plasma ließen sich im Vergleich zu fT4 deutlich seltener beobachten (55 von 613). Zudem waren 13 Urinmetabolite signifikant mit fT3 assoziiert. Die mittels 1H-NMR-Spektroskopie durch-geführte Analyse der Lipoproteinsubfraktionen zeigte positive Assoziationen zwischen fT3 und kleinen LDL-Unterklassen auf.
Die vorliegende Studie zeigte eine umfangreiche Signatur von Metaboliten auf, deren Konzentrationen im Plasma mit Serumspiegeln von fT4 und fT3, aber nicht mit TSH assoziiert waren. Somit deutet sie auf die besondere Relevanz von fT4 Spiegeln in der Therapie von Schilddrüsenerkrankungen hin, um eine ausreichende Versorgung peripherer Gewebe mit Schilddrüsen-hormonen zu gewährleisten.
Modern space missions depend more and more on electric propulsion devices for in-space
flights. The superior efficiency by ionizing the feedgas and propelling them using electric
fields with regard to conventional chemical thrusters makes them a great alternative. To
find optimized thruster designs is of high importance for industrial applications. Building
new prototypes is very expensive and takes a lot of time. A cheaper alternative is to rely
on computer simulations to get a deeper understanding of the underlying physics. In order
to gain a realistic simulation the whole system has to be taken into account including the
channel and the plume region. Because numerical models have to resolve the smallest time
and spatial scales, simulations take up an unfeasible amount of time. Usually a self-similarity
scaling scheme is used to greatly speed up these simulations. Until now the limits of this
method have not been thoroughly discussed. Therefore, this thesis investigates the limits
and the influence of the self-similarity scheme on simulations of ion thrusters. The aim
is to validate the self-similarity scaling and to look for application oriented tools to use
for thruster design optimization. As a test system the High-Efficiency-Multistage-Plasma
thruster (HEMP-T) is considered.
To simulate the HEMP-T a fully kinetic method is necessary. For low-temperature plasmas,
as found in the HEMP-T, the Particle-in-Cell (PIC) method has proven to be the best
choice. Unfortunately, PIC requires high spatial and temporal resolution and is hence
computationally costly. This limits the size of the devices PIC is able to simulate as well
as limiting the exploration of a wider design space of different thrusters. The whole system
is physically described using the Boltzmann and Maxwell equations. Using these system
of equations invariants can be derived. In the past, these invariants were used to derive a
self-similarity scaling law, maintaining the exact solution for the plasma volume, which is
applicable to ion thrusters and other plasmas. With the aid of the self-similarity scaling
scheme the computation cost can be reduced drastically. The drawback of the geometrical
scaling of the system is, that the plasma density and therefore the Debye length does not
scale. This expands the length at which charge separation occurs in respect to the system
size. In this thesis the limits of this scaling are investigated and the influence of the scaling
at higher scaling factors is studied. The specific HEMP-T design chosen for these studies is
the DP1.
Because the application of scaling laws is limited by the increasing influence of charge separation with increased scaling, PIC simulations still are computationally costly. Another approach to explore a wider design space is given using Multi-Objective-Design-Optimization
(MDO). MDO uses different tools to generate optimized thruster designs in a comparatively
short amount of time. This new approach is validated using the PIC method. During this
validation the drawback of the MDO surfaces. The MDO calculations are not self-consistent
and are based on empirical values of old thruster designs as input parameters, which not
necessarily match the new optimized thruster design. By simulating the optimized thruster
design with PIC and recalculate the former input parameters, a more realistic thruster design is achieved. This process can be repeated iteratively. The combination of self-consistent
PIC simulations with the performance of MDO is a great way to generate optimized thruster
designs in a comparatively short amount of time. The proof of concept of such a combination
is the pinnacle of this thesis.
Ex vivo- und in vivo-Untersuchungen der Anwendung von nicht-thermischem Plasma zur Blutkoagulation
(2021)
Die steigende Inzidenz und Prävalenz von Vorhofflimmern mit dem gleichzeitig erhöhten Risiko thrombembolischer Ereignisse macht eine Antikoagulation in einer immer größer werdenden Population nötig [1-3]. Das intraoperative Blutungsmanagement stellt bei Patienten, welche eine Antikoagulation erhalten, eine Schwierigkeit dar [4, 5]. Insbesondere für die direkten oralen Antikoagulantien sind Antidote häufig nicht verfügbar oder kostenintensiv [6, 7]. Die aktuell verwendete elektrische Kauterisation geht mit dem Risiko der Bildung von Nekrosen einher, welche unter Umständen zu Nachblutungen, Strikturen oder Perforationen führen können [8, 9]. Dies untermauert den Bedarf an neuen sicheren Techniken zur intraoperativen Hämostase. Eine mögliche Alternative scheint nicht-thermisches Plasma darzustellen [10]. Dies ist ein energiereiches Gas, welches eine Reihe reaktiver Komponenten enthält und eine gewebeschonende Anwendung am Menschen ermöglicht [11].
In der vorliegenden Arbeit wurde demonstriert, dass nicht-thermisches Plasma des gut charakterisierten kINPen MEDs [11] ex vivo eine Blutkoagulation im murinen Blut induzieren kann. Hierbei spielt vor allem die direkte Aktivierung der Thrombozyten eine Rolle. Nachweise der plasmatischen Gerinnung konnten ex vivo nicht gezeigt werden. Während einer murinen Leberteilresektion wurde in der vorliegenden Arbeit in nativen und Rivaroxaban-antikoagulierten Tieren eine suffiziente Blutungskontrolle durch nicht-thermisches Plasma erzielt, welche mit der elektrischen Kauterisation vergleichbar war. Weiterhin war das nicht-thermische Plasma der elektrischen Kauterisation dahingehend überlegen, als dass es zu keiner akuten Schädigung des umliegenden Gewebes und keiner zeitversetzten Nachblutung geführt hat. Die histologischen Analysen der mit nicht-thermischem Plasma behandelten Wunden zeigten die Ausbildung eines Blutkoagulums, welches am ehesten der natürlichen Koagulation entsprach. Nach Inhibition der Thrombozyten-Funktion durch Clopidogrel war das nicht-thermische Plasma in vivo nicht in der Lage, eine suffiziente Hämostase zu induzieren. Daher konnten die Thrombozyten auch in vivo als wichtige Regulatoren der durch nicht-thermisches Plasma vermittelten Hämostase herausgearbeitet werden.
Auf der Basis einer ausführlichen Literaturrecherche wurde weiterhin die Hypothese aufgestellt, dass vor allem Reduktions-Oxidations-Reaktionen an der durch nicht-thermisches Plasma induzierten Blutkoagulation beteiligt sind. In folgenden Arbeiten sollte darauf hingearbeitet werden, den Mechanismus weiter zu verstehen und effizienter zu gestalten, um dieser Methode einen Einsatz in der Zukunft der Medizin zu ermöglichen.
Die initiale Integration von Implantaten ist von hoher Bedeutung für die spätere Stabilität und
Standzeit von beispielsweise Endoprothesen im Körper. Mit Hinblick auf die steigende Zahl
von Patienten, die ein Implantat benötigen, ist es von großer Bedeutung unterschiedliche
Implantatmaterialien und Oberflächenmodifizierungen bezüglich ihrer Eigenschaften und
Interaktionen mit dem Implantatlager zu untersuchen, um diese verbessern zu können.
Ziel der vorgestellten Arbeit war die Entwicklung und Etablierung eines Screeningmodells zur
Analyse der Auswirkung von verschiedenen Metallimplantaten auf die Mikrozirkulation in
unmittelbarer Nähe des Implantats.
Dazu wurde ein neues in vivo Modell an der Chorioallantoismembran des Hühnerembryos
entwickelt, angewendet und etabliert. Dieses stellt eine Modifikation des seit Jahrzehnten
etablierten HET-CAM (Hühnereitest an der Chorioallantoismembran) dar und ermöglicht
quantitative und qualitative intravitalmikroskopische Aussagen über die Funktionelle
Gefäßdichte (FGD) und die Leukozyten-Endothel-Interaktion (LEI).
Zunächst wurden im Zuge der Modellanwendung Nickel- und Titan-Implantate verglichen, um
die mögliche Reaktionsbreite des Modells zu untersuchen. Es folgte eine Etablierung des
Modells, indem die Oberfläche der Implantate kurz vor der Applikation mit kaltem
Atmosphärendruckplasma (CAP) behandelt wurde. Die intravitalmikroskopische
Untersuchung erfolgte jeweils 24 h nach Applikation.
Die Chorioallantoismembran der mit Nickel-Implantaten behandelten Hühnerembryonen
zeigte im Vergleich zur Titan- und der internen Kontrollgruppe eine signifikante Reduktion der
FGD sowie eine signifikante Erhöhung der LEI gegenüber der Kontrollgruppe. Durch
Vorbehandlung der Nickel-Implantate mit CAP konnte der Negativeffekt auf das Gefäßsystem
signifikant reduziert werden. Für Titanimplantate konnte mit Hinblick auf die FGD kein
zusätzlicher Effekt nach der Behandlung mit CAP detektiert werden.
Die vorgestellte Arbeit zeigt, dass sich das neue Modell als Screeningmodell dazu eignet, neue
Implantatmaterialien und Oberflächenmodifikationen an der Schwelle zwischen in vitro
Zellkultur und in vivo Tiermodellen zu untersuchen. Somit könnte es dabei helfen,
Tierversuche gezielter einzusetzen. Vorteile und Einschränkungen des Modells werden
diskutiert.
The here presented dissertation investigated the molecular mechanisms, by which the food industry model bacteria Pseudomonas fluorescens and Listeria monocytogenes, grown either as planktonic cultures, were inhibited by plasma treated water (PTW) produced by a microwave-induced plasma source (MidiPLexc). As a starting point, optimal operating parameters were determined with 5 standard liters per minutes(slm)compressed air during the treatment of 10 ml deionized water within a treatment time of up to 15 min (pre-treatment time). Treatment times of 1, 3 and 5 min were selected (post-treatment time). In addition to physical parameters, i.e. temperature measurements at different spots at the plasma source during the production of the PTW, the chemical composition of PTW was determined by pH measurements, chronoamperometry (determination of the H2O2 concentration), ion chromatography (determination of the NO2-, NO3- and ONOO- concentrations) and mass spectrometry (qualitative determination of the molecules). In addition, concentration changes of reactive species over a period of 3 h indicated a decrease of the NO2- concentration as well as an increase of the NO3- and ONOO- concentration in the PTW. Microbiological assays, i.e. quantification of colony-forming units (CFU), fluorescence and XTT assays, revealed a significant reduction of the proliferation ability of the cells, membrane damages and metabolic activity have been demonstrated for planktonic cultures as well as mono- and multispecies biofilms. PTW effects on biofilm structures were investigated using microscopic methods such as fluorescence microscopy, confocal laser scanning microscopy (CLSM), atomic force microscopy (AFM), and scanning electron microscopy (SEM), as well as physical methods such as contact angle measurements. Significant changes in the biofilm structure have been shown, which indicate an ablation of the biofilm mass from top to bottom by approximately 2/3 of the biofilm mass and a destruction of the extracellular matrix (ECM) by the reactive species within the PTW. Subsequently, fresh-cut lettuce has been treated with PTW produced by up-scaled plasma sources. Apart from qualitative parameters of the lettuce after PTW treatment such as texture and color, the concentration of PTW reactive species have been determined. These experiments showed that the composition of the reactive species were slightly different from that of the laboratory-scaled plasma source MidiPLexc. Notably, the PTW treatment did not cause significant changes in texture and color of the fresh-cut lettuce. Finally, a synergistic effect of PTW treatment followed by plasma-processed air (PPA) drying was demonstrated application-specific.
In this work, studies with respect to the exhaust problem were performed
in the stellarator experiment Wendelstein 7-X with different target concepts and different magnetic field geometries. Different infrared cameras were used to study the heat flux from the plasma onto the PFC. In the first publication, the limiter set-up was used with a simpler magnetic topology in the plasma edge. The radial fall-off of the parallel heat flux for inboard limiters in W7-X shows, similar to inboard limiters in tokamaks, two different radial fall-off lengths, a short (narrow) one, characterizing the near-SOL, and a long (broad) characterizing the far-SOL. For the far-SOL, the heating power and connection length have been identified as the main scaling parameters, while for the near-SOL, the electron temperature close to the LCFS has been identified as the main scaling parameter. The two fall-off lengths differ by a factor 10, and the found scalings for both regimes differ from known models and experimental scalings in tokamaks. A turbulent-driven feature was discussed in the publication as a possible explanation for the behavior of the fall-off length in W7-X.
The gained information and data have been further used to support many
other publications, covering the symmetry of the heat loads, the
energy balance of the machine, and seeding experiments.
The heat exhaust in W7-X with an island divertor was studied in the second
and third publication. Definitions of parameters such as peaking factor and
wetted area were applied for the heterogeneous heat flux pattern on the
W7-X divertor. It was shown that the island divertor concept is capable
of spreading out the heat efficiently, resulting in large wetted areas of up to 1.5 m2. The reached values for the wetted area are comparable to the ones of the larger tokamak JET but with a much smaller ratio of wetted
area to the area of the last closed flux surface. Furthermore, a positive
scaling of the wetted area with the power in the SOL was observed. This
scaling is beneficial for future reactors but needs further investigation of the involved transport processes. The peaking factor (discussed in the second publication) describes how concentrated the heat load is within the region of the strike line. It was shown that this factor is decreasing for increasing densities without affecting the wetted area. The present work paves the way for further analysis of the transport processes of the heat flux towards the island divertor of Wendelstein 7-X.
The active screen plasma nitrocarburizing (ASPNC) technology is a state-of-the-art plasma-assisted heat treatment for improving surface hardness and wear resistance of metallic workpieces based on thermochemical diffusion. In comparison to conventional plasma nitrocarburizing, the use of an active screen (AS) improves thermal homogeinity at the workload and reduces soot formation. Further it can serve as a chemical source for the plasma processes, e.g. by use of an AS made of carbon-fibre reinforced carbon. This compilation of studies investigates the plasma-chemical composition of industrial- and laboratory-scale ASPNC plasmas, predominantly using in-situ laser absorption spectroscopy with lead-salt tuneable diode lasers, external-cavity quantum cascade lasers, and a frequency comb. In this way the temperatures and concentrations of the dominant stable molecular species HCN, NH3, CH4, C2H2, and CO, as well as of less prevelant species, were recorded as functions of e.g. the pressure, the applied plasma power, the total feed gas flow and its composition. Additionally, the diagnostics were applied to a chemically similar plasma-assisted process for diamond deposition.
Resulting from this thesis are new insights into the practical application of an AS made of CFC, the plasma-chemistry involving hydrogen, nitrogen, and carbon, and the particular role of CO as an indicator for reactor contamination. The effect of the feed gas composition on the resulting nitrogen- and carbon-expanded austenite layers was proven by combination of in-situ laser absorption spectroscopy with post-treatment surface diagnostics. Furthermore this work marks the first use of frequency comb spectroscopy with sub-nominally resolved Michelson interferometry for investigation of a low-pressure molecular discharge. This way the rotational bands of multiple species were simultaneously measured, resulting in temperature information at a precision hitherto not reached in the field of nitrocarburizing plasmas.
Background: Hyperthyroidism is known to induce a hypercoagulable state. It stimulates plasma levels of procoagulative factors and reduces fibrinolytic activity. So far most of the data have been derived from patients with endogenous hyperthyroidism with a wide variability in the underlying pathogenesis and severity of the disease. Objectives: In this study we experimentally induced thyrotoxicosis in healthy volunteers to explore the effects of thyroxine excess on the plasma proteome. Using a shotgun proteomics approach, the abundance of plasma proteins was monitored before, during and after thyrotoxicosis. Methods: Sixteen healthy male subjects were sampled at baseline, 4 and 8 weeks under 250 µg/day thyroxine p.o., as well as 4 and 8 weeks after stopping the application. Plasma proteins were analyzed after depletion of 6 high-abundance proteins (MARS6) by LC-ESI-MS/MS mass spectrometry. Mass spectrometric raw data were processed using a label-free, intensity-based workflow. Subsequently, the linear dependence between protein abundances and fT<sub>4</sub> levels were calculated using a Pearson correlation. Results: All subjects developed biochemical thyrotoxicosis, and this effect was reversed within the first 4 weeks of follow-up. None of the volunteers noticed any subjective symptoms. Levels of 10 proteins involved in the coagulation cascade specifically correlated with fT<sub>4</sub>, supporting an influence of thyroid hormone levels on blood coagulation even at nonpathological levels. Conclusions: The results suggest that experimental thyrotoxicosis exerts selective and specific thyroxine-induced effects on coagulation markers. Our study design allows assessment of thyroid hormone effects on plasma protein levels without secondary effects of other diseases or therapies.
The importance of ion propulsion devices as an option for in-space propulsion of space
crafts and satellites continues to grow. They are more efficient than conventional chemi-
cal thrusters, which rely on burning their propellant, by ionizing the propellant gas in a
discharge channel and emitting the heavy ions at very high velocities. The ion emission
region of a thruster is called the plume and extends several meters axially and radially
downstream from the exit of a thruster. This region is particularly important for the effi-
ciency of a thruster, because it determines energy and angular distribution of the emitted
ions. It also determines the interaction with the carrier space craft by defining the electric
potential shape and the fluxes and energies of the emitted high energy ions, which are the
key parameters for sputter erosion of satellite components such as solar panels. Developing
new ion thrusters is expensive because of the high number of prototypes and testing cycles
required. Numerical modeling can help to reduce the costs in thruster development, but
the vastly differing length and time scales of the system, particularly the large differences of
scales between the discharge chamber and the plume, make a simulation challenging. Often
both regions are considered to be decoupled and are treated with different models to make
their simulation technically feasible. The coupling between channel and plume plasmas and
its influence on each other is disregarded, because there is no interaction between the two
regions. Therefore, this thesis investigates the physical effects which arise from this cou-
pling as well as models suitable for an integrated simulation of the whole coupled problem
of channel and plume plasmas. For this purpose the High Efficiency Multistage Plasma
Thruster (HEMP-T) ion thruster is considered.
For the discharge channel plasma, a fully kinetic model is required and the Particle-in-Cell
(PIC) method is applied. The PIC method requires very high spatial and temporal resolu-
tions which makes it computationally costly. As a result, only the discharge channel and the
near-field plume close to the channel exit can be simulated. In the channel, the results show
that electrons are magnetized and follow the magnetic field lines. The orientation of the
magnetic field there is mostly parallel to the symmetry axis and the channel walls which re-
sults in a high parallel electron transport and leads to a flat electric potential and a reduced
plasma-wall sheath. Only at the magnetic cusps, which are characteristic of HEMP-Ts the
electrons are guided towards the wall, with ions following due to quasineutrality, where a
classical plasma-wall sheath develops. The ion-wall contact is thus limited to the cusp re-
gion. The small radial drop of the potential towards the wall gives rather low energies of
ions impinging at the wall and minimizes erosion in the HEMP-T.
In the near-field plume, which extends from the thruster exit plane to some centimeters
downstream, the ion emission characteristics is defined. The ratio of radial and axial elec-
tric field components in this region determines the ion emission angle which should be
minimized for maximum thruster efficiency. The plasma discharge in the channel produces
high plasma densities and the subsequent drop from plasma to vacuum potential occurs
further downstream for higher densities. This increases the ratio of radial and axial electric
field components because the plasma expands radially outside of the confinement from the
dielectric discharge channel walls. The potential structure in the near-field plume impacts
also the supply of electrons for the channel discharge because the electrons enter the channel
from the plume. An effect which arises from this coupling is the breathing mode oscilla-
tion. It is an oscillation which is observed in all plasma quantities and is located near the
thruster exit. The oscillation frequency measured in the simulation is in good agreement
with a predator-prey estimate which validates this ansatz. However, the electron tempera-
ture, assumed constant in the predator-prey model, correlates inversely with the oscillation,
i.e. it is minimal at the current maximum and vice versa, which contributes to the observed
oscillations. Because of the oscillation of the plasma number density, the potential drop also
oscillates in the exit region and thus the ratio of radial to axial electric field components,
which results in the oscillation of the mean ion emission angle.
Regarding suitable models for a combined simulation of channel and plume plasmas, the
PIC model for channel and near-field plume is explicitly coupled to a hybrid fluid-PIC
model for the plume. The latter treats the electrons as a fluid, hence increasing the effective
spatial and temporal resolutions which can be applied in the plume simulations at the cost
of reduced accuracy of the electron model. Plasma densities decrease by two orders of
magnitude two meters downstream from the channel exit. The explicitly coupled kinetic
and hybrid PIC models are well suited for the computation of a HEMP-T and its plume
expansion, but they disregard the coupling of channel and plume plasmas for which other
methods are necessary. For this purpose a new approach is presented with a proof-of-
principle validation. The limited spatial resolution in the plume can be overcome with the
mesh-coarsening method, which increases the resolution in regions of low plasma density
without numerical artifacts. Sub-cycling for the electrons in the plume can then be used
to increase the temporal resolution in the plume. The combination of both methods, called
the sub-cycling mesh-coarsening (SMC) algorithm in the scope of this work, promises high
savings in computational cost which can make a combined simulation of plume and channel
plasmas feasible.
Die Anwendung von Niedrigtemperatur-Atmosphärendruckplasmen im Bereich der
Wundversorgung gewinnt stetig an Bedeutung und so steigt das Interesse an den damit
ausgelösten biologischen Vorgängen im Organismus. Es bestehen zahlreiche Studien zum
Einfluss von Plasma auf verschiedene Zellen in Kultur. In der vorliegenden Arbeit wurde die
Wirkung von Plasma auf einen intakten Zellverband, der menschlichen Haut, umfangreich
molekularbiologisch untersucht.
Es wurde der Atmosphärendruck-Plasmajet kINPen® MED verwendet, um ex-vivo
Hautproben von insgesamt 9 Patienten zu behandeln. Mittels Fluoreszenzmikroskopie wurden die Hautbiopsien hinsichtlich Differenzierung, Proliferation, Apoptose und DNA 24 Stunden nach Plasmaexposition beurteilt. Weiterhin wurde die Sekretion von Zytokinen mittels ELISA erforscht. Die Dauer der punktuellen Plasmabehandlungen betrug 1 Minute, 3 Minuten und 5 Minuten.
Die größten Limitationen im Studiendesign waren der geringe Probenumfang sowie die
Inhomogenität der Versuchsgruppen. Es konnten keine signifikanten Unterschiede zwischen
behandelter und unbehandelter Hautprobe nachgewiesen werden. Trotz allem wurden
wichtige Tendenzen beobachtet. Die Anwendung des Plasmas scheint das grundsätzliche
Differenzierungsmuster der Epidermis kaum zu beeinflussen. Bei längerer Behandlung bis 5
Minuten stieg die Anzahl basaler apoptotischer Zellen, während es kaum Änderungen im
Auftreten von DNA Doppelstrangbrüchen sowie der Sekretion von IL6 oder IL8 gab. Die
Anzahl proliferativer basaler Zellen stieg bis zu einer Plasmaexposition von 3 Minuten.
Möglicherweise wirken kurzzeitige Plasmabehandlungen proliferationsfördernd auf
Keratinozyten. Dies könnte eine weitere Erklärung für den positiven Einfluss von Plasma auf
die Heilung von Wunden sein. Längere Behandlungen lösen womöglich Apoptosen aus,
jedoch ohne DNA Schäden herbeizuführen.
Um Nebenwirkungen zu minimieren, bedeutet dies für die klinische Praxis, möglichst kurze
Expositionszeiten einzuhalten. Um eine optimale therapeutische Anwendung
unterschiedlicher Plasmaquellen, die sich in Zusammensetzung und Intensität unterscheiden,
zu ermöglichen, sind weitere Studien bezüglich Behandlungszeit und entsprechender
biologischer Wirkung notwendig.
Wichtige Ergebnisse dieser Arbeit sind in die Publikation von Hasse et al. eingeflossen
(Hasse et al. 2016).
In dieser Arbeit wurden die Eigenschaften von atmosphärendruckplasmaaktivierten Natriumchloridlösungen (NaCl-Lösungen), unter Anwendung von nass-chemischen und mikrobiologischen Analysenverfahren, untersucht. Es zeigte sich, dass plasmaaktivierte NaCl-Lösungen sowohl mit kurzzeitigen als auch mit langzeitigen antimikrobiellen Effekten generiert werden können. Diese Effekte korrelieren mit einer Änderung der chemischen Zusammensetzung der flüssigen Phase. Molekularbiologische Untersuchungen zeigten, dass die antimikrobiellen Effekte auf unterschiedlichen Wirkmechanismen, vor allem auf oxidativem und nitrosativem Stress, beruhen. Anwendungsorientierte Untersuchungen haben gezeigt, dass plasmaaktivierte NaCl-Lösungen über ein enges Wirkspektrum (grampositive und gramnegative Erreger) verfügen, sich keine schnellen Resistenzen gegen den Testorganismus ausbilden und eine Kombination mit handelsüblichen Antibiotika ein vielversprechender Ansatz für eine Wirkungssteigerung der verwendeten Antibiotika ist.
Manipulating and utilizing plasmas becomes a more and more important task in various research fields of physics and in industrial developments. Especially in nowadays spacerelevant applications there are different ideas to modify plasmas concerning particular tasks.
One major point of interest is the ability to influence plasmas using magnetic fields. To study the underlying physical effects that were achieved by these magnetic fields for both scenarios Particle-in-Cell simulations were done. Two examples are discussed in this thesis.
The first example originates from an experiment performed by the European Space Agency ESA in collaboration with the German Space Agency DLR. To verify the possibility of heat-flux reduction by magnetic fields onto the thermal protection system of a space vehicle a simplified experiment on earth was developed. Most of the heat that is created during re-entry comes from compression of the air ahead of the hypersonic vehicle, as a result of the basic thermodynamic relation between temperature and pressure. The shock front, which builds up in front of the vehicle deflects most of the heat and prohibits the surface of the space vehicle from direct contact with the maximum flux. State of the art spacecrafts use highly developed materials like ceramics to handle the enormous heat. An attractive approach to reduce costs is to use magnetic fields for heat-flux reduction. This would allow the use of cheaper materials and thus reduce costs for the whole space mission. A partially-ionized Argon beam was used to create a certain heat-flux onto a target. The main finding of the experimental campaign was a large mitigation of heat-flux by applying a dipole-like magnetic field. The Particle-in-Cell method was able to reproduce experimental observations like the heat-flux reduction. An additionally implemented optical diagnostics module allowed to confirm the results of the spectroscopy done during the experiment. The underlying effect that is responsible for the heat-flux reduction was identified as a coupling between the modified plasma and the dominating neutral flux component. The plasma, that is guided towards the target, act as a shield in front of the target surface for arriving neutrals. These neutrals are slowed down by charge-exchange collisions. Furthermore the magnetic field induces an increased turbulent transport that is also needed to reach a reduction in heat-ux. The turbulent transport was also obtained by three-dimensional Direct Simulation Monte Carlo simulations. Unfortunately, such source driven turbulence can not be expected in space, so that a heat flux reduction in real space applications is questionable. Nevertheless, other effects like the induced turbulence by the rotating vehicle can compensate the missing source driven effect.
The second scenario in which a magnetic field is used to modify the heat flux of a plasma is the operation of the pulsed cathodic arc thruster. The same Particle-in-Cell code was used to simulate a typical pulse of this newly developed thruster of Neumann Space Pty Ltd. The typical behavior of the thruster could be reproduced numerically. The thrust is mainly produced by fast electrons. These electrons are accelerated by electric fields as a result of a plasma-beam instability. This plasma-beam instability was verified by a phase space diagnostics for the electrons. To demonstrate the influence of the magnetic field a simulation of the cathodic arc thruster without magnetic field and one with magnetic field were compared. It was shown that the use of a magnetic field leads to a ten times larger thrust by directing the heat ux. The resulting narrow plume is an additional Advantage of the particle guiding magnetic field. This narrowness of the plume reduces the danger of interaction with other components of the space vehicle.
Both scenarios demonstrate the different capabilities for electromagnetic fields to manipulate plasmas and especially the corresponding heat-flux with respect to certain tasks. The possibilities range from reducing the heat-flux onto a target to maximizing the thrust by directing the heat-ux. This thesis demonstrates that simulations are a great tool to support experiments and to deliver an improved physics understanding. They help to identify the basic physics principles in the different systems, because they can deliver information not accessible to experiments.
In particular, a better understanding of the influence of electromagnetic fields on the heat-flux distribution in space-relevant applications was obtained. This can be the basis for further simulation-guided optimization, e.g. for the design of more effective cathodic arc thrusters. Here, the goal is to minimize costs for prototypes by replacing the hardware by virtual prototypes in the simulations. This allows to test basic design ideas in advance and get more highly-optimized designs at a fraction of time and costs.
Gegenstand der hier vorgestellten Arbeit ist die Beschichtung von Wundauflagen mit Zinkoxid- und Silberhaltigen antibakteriellen Schichten. Die Aufbringung der Schichten erfolgt dabei auf den Wundauflagen mittels Atmosphärendruckplasma. Die Matrix der Schichten besteht aus Siliziumdioxid, in welcher die Wirkstoffe eingelagert sind. Auf diesem Weg hergestellten Wundauflagen wurden hinsichtlich ihrer antibakteriellen Wirkung und zytotoxischen Eigenschaften charakterisiert. Ziele waren ein minimaler Einsatz an Wirkstoffen und die Nutzung eines modernen Beschichtungsverfahrens. Der zytotoxische Einfluss der Wundauflagen wurde an 3D-Hautmodellen im Vergleich zu den am Markt befindlichen Produkten validiert.
The thyroid as the largest endocrine gland mainly produces and secretes the thyroid hormones (TH): 3,3’,5-triiodo-L-thyronine (T3) and its pro-hormone L-thyroxine (T4). Besides the impact on growth, normal development, bone marrow structure, the cardiovascular system, body weight and thermogenesis, TH play a vivid role in many metabolic regulatory mechanisms in almost all tissues. Thyroid diseases are relatively prevalent and cause, due to the resulting TH imbalances, a broad spectrum of effects. Many of them manifest in pathologically increased or decreased TH levels defined as hyperthyroidism or hypothyroidism, respectively. Routinely, determination of the thyroid state is based on the assessment of the classical markers TSH and free T4. However, this practice has several drawbacks. Moreover, elucidation of the pleiotropic effects of TH on multiple molecular pathways is mostly based on cell culture, tissue and rodent models. Analysis of animal biofluids like serum and urine using metabolomics approaches demonstrated the extensive impact of TH on other body compartments. In contrast, proteome profiling has not been exploited for the comprehensive characterization of the general metabolic effects of TH. Plasma as a large and diverse compartment of the human proteome provides a great opportunity to identify novel protein markers of thyroid function as well as to characterize metabolic effects of TH in humans.
Therefore, a study of experimental thyrotoxicosis was performed with 16 male volunteers treated with 0.25 mg/d levothyroxine (L-T4) for 8 weeks to induce a hyperthyroid state. Plasma samples were collected before the L-T4 application started, two times during the treatment and additionally two times after withdrawal. Proteome analysis revealed remarkable alterations including increased levels of two known proteins known to correlate with TH levels (sex hormone-binding globulin and cystatin C). The correlation with free T4 levels revealed 76 out of 437 detected proteins with a Pearson correlation coefficient of r ≥ |0.9|. One prominent signature included 10 coagulation cascade proteins exhibiting significantly increased plasma levels during thyrotoxicosis, thereby revealing a trend towards a hypercoagulative state in hyperthyroidism. To overcome the statistical drawbacks of the Pearson correlation analysis, additionally a mixed-effect linear regression model using serum free T4 concentrations as exposure and protein abundances as outcome while controlling for age, BMI, and batch was implemented. Application of this model resulted in the detection of 63 proteins with significant associations to free T4 levels. Besides the already mentioned augmented coagulation, a significant drop in the amounts of three apolipoproteins (ApoD, ApoB-100 and ApoC3) was observed. Furthermore, an increased abundance of proteins assigned to the complement system was detected.
Experimental studies in humans were complemented by corresponding analyses in murine models. In the current work, plasma samples of two murine studies including male C57BL/6 wildtype mice were analyzed to elucidate the impact of thyroid dysfunction on the plasma proteome. The first study was similarly designed as the human model of experimentally induced thyrotoxicosis and assigned the animals to three groups: a control group, a T4 treatment group, and a T4 recovery group, whereupon the latter first received T4 followed by a subsequent TH normalization period. A high proportion of plasma proteins exhibited significantly different protein levels during T4 application (n = 120), where 90 of these also showed a corresponding reverse trend after T4 withdrawal (T4 recovery vs. T4), thereby displaying transient alterations. The molecular pattern of hyperthyroidism in the murine model indicated, as in the human study, a pronounced decrease in apolipoproteins. However, in clear contrast to the human data, the levels of proteins related to the coagulation cascade and complement system were also transiently decreased in mice, while being increased in humans.
The second murine analysis focused on the impact of hyper- and hypothyroidism caused by T3 or T4 treatment and MMI/KClO4 application, respectively. In general, compared to the first murine study less clear alterations of protein levels were detected. Proteins related to the complement system revealed fewer changes in the T3 group and only marginal changes after T4 induction. Unexpectedly, the MMI/KClO4-induced hypothyroidism caused a reduction of the levels of several proteins assigned to the complement system, although different components and factors were affected.
Generally, rodent studies partially provided a divergent picture of TH action as compared to human studies. However, in spite of inconsistent results in studies regarding the effects of TH that are possibly due to species-specific differences, an important role of TH on several metabolic and other pathways, e.g. in the process of blood coagulation and apolipoprotein regulation, is evident. The results from both murine and human studies presented here provide novel insights into changes in the plasma proteome in the context of thyroid diseases which might contribute to a better understanding of TH action on metabolism and other pathways.
Das fortgeschrittene, metastasierte Pankreaskarzinom stellt allen Fortschritten innerhalb der Onkologie zum Trotz weiterhin eine Diagnose mit infauster Prognose dar, deren palliative Therapiemöglichkeiten ebenfalls nicht zufriedenstellend sind. Seit einigen Jahren besteht die Hoffnung den vierten Aggregatzustand in Form von ‚nicht-thermischem Plasma' (NTP) in der modernen Tumortherapie einzusetzen. Dies beruht auf der Generierung zahlreicher reaktiver Sauerstoff- und Stickstoffspezies, die in der Balance aus Wachstum und Apoptose von Tumoren eine entscheidende Rolle einnehmen. In Zusammenschau aller im Rahmen dieser Arbeit erhobenen in vitro Ergebnisse und der hierzu einsehbaren Literatur lässt sich eine selektive, anti-tumoröse Wirkung von NTP festhalten, die sich in reduzierter Zellviabilität und -proliferation, sowie effektiver Apoptoseinduktion ohne Bildung von Nekrosen äußert. Diese Effekte werden vorrangig über im Medium gelöste reaktive Sauerstoff- und Stickstoffspezies vermittelt, sodass auch zellfreie, NTP-behandelte Flüssigkeit diese Wirkung erzielt. In einem syngenen Mausmodell einer Peritonealkarzinose des Pankreaskarzinoms konnten die antiproliferativen und proapototischen Effekte dieser indirekten NTP-Behandlung nachgestellt werden. Die repetitive intraperitoneale Applikation resultierte in einer signifikanten Reduktion der Tumoren hinsichtlich Anzahl, Größe und Gewicht. Dabei zeigte sich eine beachtliche effektive Eindringtiefe innerhalb der Tumorläsionen. Lokale oder systemische Nebenwirkungen konnten unter der Therapie nicht beobachtet werden, insbesondere wiesen die übrigen aufgearbeiteten intraperitonealen Gewebe keine makro- oder mikroskopisch sichtbaren Veränderungen auf und auch die Blutzusammensetzung zeigte sich unverändert gegenüber der Kontrollgruppe. In dieser Arbeit wurde zudem - nach Kenntnisstand des Autors - erstmals der Einfluss einer indirekten NTP-Behandlung auf das Überleben immunkompetenter, Tumor-tragender Mäuse untersucht und hierbei ein signifikanter Überlebensvorteil demonstriert.
Die präsentierte Arbeit stellt einen wichtigen Schritt in der Entwicklung neuer Therapieoptionen des metastasierten Pankreaskarzinoms dar, als dass die selektive in vitro Wirksamkeit von NTP nun auch in vivo in einem komplexen Organismus wie der immunkompetenten Maus nachgestellt werden konnte. Künftige Arbeiten zu den NTP-Regulationsmöglichkeiten durch Flüssigkeits- und Plasmamodifikationen werden mutmaßlich das vollständige Potential dieses neuartigen Therapieansatzes offenbaren.
The content of this thesis can be summarized as follows: (i) The deposition processes of SiOx and SiOxCyHz coatings were investigated in a low-pressure, low temperature HMDSO-O2-N2 plasmas. Infrared laser absorption spectroscopy (IRLAS) and optical emission spectroscopy (OES) were combined to measure the gas temperatures in the hot and colder zones of the plasma as well as to monitor the concentration of the methyl radical, CH3, and of seven stable molecules, HMDSO, CH4, C2H2, C2H4, C2H6, CO and CO2. Tunable lead salt diode lasers (TDLs) and an external-cavity quantum cascade laser (EC-QCL) were simultaneously employed as radiation sources to perform the IRLAS measurements. They were found to be in the range between 10^{11} to 10^{15} cm^{−3}. The influence of the discharge parameters of power, pressure and gas mixture on the molecular concentrations was studied. The plasma generation is characterized by a certain degree of inhomogeneity with different temperature zones, i.e., hottest, hot and colder zones depending on the construction of the reactor. This complexity is characterized by the multiple molecular species including the HMDSO precursor and products in ground and excited states existing in the plasma. (ii) Employing similarly IRLAS and OES techniques, the deposition of nanocrystalline diamond at relatively low temperature in low-pressure MW H2 plasmas with small ad-mixtures of methane and carbon dioxide was investigated. Five methods were applied for an extensive temperature analysis, providing new insights into energetic aspects of the multi-component non-equilibrium plasma. The OES method provided information about the gas temperature of H2 inside the MW plasma. Using lead salt diode lasers, the rotational temperature of the methyl radical, CH3 , and gas temperature of methane molecule, CH4 , was measured. A variety of CO lines in the ground and in three excited states have been analysed using an EC-QCL with a relatively wide spectral range. These methods have shown that based on the construction of the DAA reactor using 16 single plasma sources the plasma generation is characterized by a variety of hottest, hot and colder zones. Extensive measurement of these various species temperatures in the complex plasma enabled the concentration determination of the various stable and unstable plasma species, which were found to be in the range between 10 11 to 10 15 cm −3 . The influence of the discharge parameters, power and pressure, on the molecular concentrations has been studied. To achieve insight into general plasma chemical aspects, the dissociation of the carbon precursor gases including their fragmentation and conversion to the reaction products was analysed in detail. The evolution of the concentration of the methyl radical, CH 3 , of five stable molecules, CH4, CO2, CO, C2H2 and C2H4, and of vibrationally excited CO in the first and second hot band was monitored in the plasma processes by in situ infrared laser absorption spectroscopy using lead salt diode lasers (TDL) and an external-cavity quantum cascade laser (EC-QCL) as radiation sources. OES was applied simultaneously to obtain complementary information about the degree of dissociation of the H2 precursor gas. The analysis of the carbon and oxygen mass balances shows clearly, that the deposition on the reactor walls and the production of other hydrocarbons species may act as sinks for carbon and oxygen. (iii) The absolute line strengths of many P-branch transitions of the ν3 fundamental of {28}^SiH4 were determined using the wide tuning range and the narrow line width of a cw EC-QCL between 2096 and 2178 cm^{−1}. The line positions and line strengths of transitions of the stretching dyad within the P-branch of {28}^SiH4 were determined with an estimated experimental measurement accuracy of 10%. The high spectral resolution available has enabled us to resolve and measure representative examples of the tetrahedral splittings associated with each component of the P-branch. The positions of these components are in excellent agreement with spherical top data system (STDS) predictions and theoretical transitions from the TDS spectroscopic database for spherical top molecules. To our knowledge, this is the first reported measurement of these line strengths in this band and is an example of the applicability of high-powered, widely tunable EC-QCLs to high resolution spectroscopy in the MIR. (iv) Similarly, the determination of the silyl radicals, ν3 band, line strengths is ongoing using the same cw EC-QCL. This effort was impaired by silane and other unknown species lines overlap; however, the silyl radicals was successfully detected in a SiH4/H2 plasma. A method to determine the silyl line strengths has been presented through its iterative decay measurements which relied on the value of the silyl radical self reaction constant. There was a consensus of its value in the literature.
The aim of this thesis is to concentrate on the investigation of these ROS&RNS composition distribution and their production pathways in the gas phase produced by a plasma jet. By understanding the physical mechanisms behind the generation of the ROS&RNS a precise tuning and design of the composition distribution in the gas phase can be achieved. One crucial physical parameter is the dissipated power inside the plasma. Only if this parameter is known a meaningful comparison of different feed gas settings is possible. Therefore, a concept for measuring the dissipated power inside the plasma for the modified micro-scaled atmospheric pressure plasma jet( µAPPJ) is designed. Additionally, due to achievements within this thesis it is now possible to ignite a homogeneous discharge in argon and helium within the geometry of the µAPPJ. The used feed gas is a determining factor concerning the electron energy distribution function and consequently influencing the production mechanism of the ROS&RNS. First of all, the electrical characterisation of the modified µAPPJ was performed including the alpha-to-gamma transition. It is shown that the alpha-to-gamma transition power is increasing with increasing frequency. For the first time it is now feasible to investigate the influence of the dissipated power on the neutral gas temperature, the metastable atom densities and the ROS&RNS production for the modified µAPPJ with argon and helium as feed gas. Due to the possibility of changing the feed gas and controlling the dissipated power a fundamental insight into the production mechanism of the ROS&RNS generated by the plasma jet is achieved. With rising dissipated power the temperature and the metastable densities as well as the ozone and nitrogen dioxide concentrations are increasing. By adding molecular oxygen and nitrogen to the feed gas of a plasma jet the ROS&RNS composition can be tuned. However, also the dissipated power is changed by the small amount of admixtures. Due to the developed dissipated power measurements within this thesis it was possible to disentangle the influence of the admixture on the power and on the ROS&RNS production. If the dissipated power is fixed for the µAPPJ with argon and helium feed gas, respectively, the highest amount of ozone was measured with oxygen admixture in an argon discharge, the highest amount of dinitrogen pentoxide with nitrogen admixture in an argon discharge and the highest amount of nitrogen dioxide with nitrogen admixture in a helium discharge. Beyond the influence of the dissipated power and the molecular admixture on the ROS&RNS production the feed gas temperature is a crucial parameter for the corresponding chemical reactions. By changing this parameter the distribution of ozone and nitrogen dioxide can be tuned precisely in such a way that with increasing temperature the ozone density goes down and the nitrogen dioxide density rises. Another determinant for the ROS&RNS composition produced by an atmospheric pressure plasma jet is the influence of ambient air. If the ambient air is changing from pure nitrogen to pure oxygen atmosphere the ozone density produced by the plasma jet is increasing. For the same conditions the nitrogen dioxide has a maximum at an oxygen-to-nitrogen ratio of 1:1. To avoid the influence of the ambient air on the reactive species production the afterglow of the µAPPJ was prolonged with a glass tube. By increasing the amount of molecular admixtures to the feed gas with each in equal quantities a totally different ROS&RNS composition can be obtained compared without the glass tube. It figures out that for small molecular admixtures the reactive species composition is nitrogen dominated and for higher admixtures it is oxygen dominated. Consequently, by shielding the ambient air from the active effluent and by admixing molecular oxygen and nitrogen the ROS&RNS composition can be designed.
The present thesis deals with dynamic structures that form during the expansion of plasma into an environment of much lower plasma density. The electron expansion, driven by their pressure, occurs on a much faster time scale than the ion expansion, owed to their mobility. The high inertia of the ions causes the generation of an ambipolar electric field that decelerates the escaping electrons while accelerating the ions. The ambipolar boundary propagates outwards and forms a plasma density front. For a small density differences, the propagation of the front can be described with the linear ansatz for ion acoustic waves. For a large density differences, experiments have shown that the propagation velocity of such a front is still related to the ion sound velocity. However, the reported proportionality factors are scattered over a wide range of values, depending on the considered initial and boundary conditions. In this thesis, the dynamics during plasma expansion are studied with the use of experiments and a versatile particle-in-cell simulation. The experimental investigations are performed in the linear helicon device Piglet. The experiment features a fast valve, which is used to shape the neutral gas density profile. During the pulsed rf-discharges, plasma is generated in the source region and expands collisionless into the expansion chamber. The computer simulation is tailored very close to the experiment and provides a deeper insight in the particle kinetics. The experimental results show the existence of a propagating ion front. Its velocity is typically supersonic and depends on the density ratio of the two plasmas. The ion front features a strong electric field. The front can have similar properties to a double layer is not necessarily a double layer by definition. The computer simulation reveals that the propagating electric field repels the downstream ambient ions. These ions form a stream with velocities up to twice as high as the front velocity. The observed ion density peak is due to the accumulation of the repelled ions and is located at their turning point. The ion front formation depends strongly on the initial ion density profile and is part of a wave-breaking phenomenon. The observed front is followed by a plateau of little plasma density variation. This could be confirmed for the expansion experiment by a comparison with virtual diagnostics in the computer simulation. The plateau has a plasma density determined by the ratio between the high and low plasma density. It consists of streaming ions that have been accelerated in the edge of the main plasma. The presented results confirm and extend findings obtained by independent numerical models and simulations.
Magnetic reconnection is a fundamental plasma process where a change in field line connectivity occurs in a current sheet at the boundary between regions of opposing magnetic fields. In this process, energy stored in the magnetic field is converted into kinetic and thermal energy, which provides a source of plasma heating and energetic particles. Magnetic reconnection plays a key role in many space and laboratory plasma phenomena, e.g. solar flares, Earth’s magnetopause dynamics and instabilities in tokamaks. A new linear device (VINETAII) has been designed for the study of the fundamental physical processes involved in magnetic reconnection. The plasma parameters are such that magnetic reconnection occurs in a collision-dominated regime. A plasma gun creates a localized current sheet, and magnetic reconnection is driven by modulating the plasma current and the magnetic field structure. The plasma current is shown to flow in response to a combination of an externally induced electric field and electrostatic fields in the plasma, and is highly affected by axial sheath boundary conditions. Further, the current is changed by an additional axial magnetic field (guide field), and the current sheet geometry was demonstrated to be set by a combination of magnetic mapping and cross-field plasma diffusion. With increasing distance from the plasma gun, magnetic mapping results in an increase of the current sheet length and a decrease of the width. The control parameter is the ratio of the guide field to the reconnection magnetic field strength. Cross-field plasma diffusion leads to a radial expansion of the current sheet at low guide fields. Plasma currents are also observed in the azimuthal plane and were found to originate from a combination of the field-aligned current component and the diamagnetic current generated by steep in-plane pressure gradients in combination with the guide field. The reconnection rate, defined via the inductive electric field, is shown to be directly linked to the time-derivative of the plasma current. The reconnection rate decreases with increasing ratio of the guide field to the reconnection magnetic field strength, which is attributed to the plasma current dependency on axial boundary conditions and the plasma gun discharge. The above outlined results offer insights into the complex interaction between magnetic fields, electric fields, and the localized current flows during reconnection.
The laser-matter interaction is a topic of current research. In this context, the interaction of intensive laser radiation with atomic clusters is of special interest. Du to the small cluster size, the laser field can penetrate the whole cluster volume, which leads to a high absorption of energy in the cluster. As a result, plasmas with high density and high temperature are produced. In the early phase of the laser-cluster interaction, free electrons are initially created in the cluster due to tunnel ionization or photoionization. Via collisions of these electrons with the cluster atoms, the ionization is increased and thus a dense nanoplasma is produced, which is heated by the laser. If free electrons leave the cluster during the laser-cluster interaction (outer ionization), a positive charge buildup is created. The associated charge repulsion finally can lead to the fragmentation of the cluster due to Coulomb explosion. Experimentally, interesting phenomena emerging from laser-excited clusters are observed, e.g., the creation of fast electrons, the production of highly charged ions, and X-ray emission. In this dissertation, the interaction of Gaussian laser pulses in the infrared regime with argon and xenon clusters is simulated by means of a nanoplasma model. Considering laser intensities in the non-relativistic regime, the relevant processes such as ionization, heating and expansion are theoretically described in this model with a set of coupled rate equations and hydrodynamic equations. One focus of the thesis is on the heating of the nanoplasma via inverse bremsstrahlung (IB), which is due to the absorption of laser photons in electron-ion collisions. In particular, the important question is investigated whether the consideration of the ionic structure – that means, the nuclear charge and the bound electrons – modifies the electron-ion collisions and thus the IB heating rate. Starting from a quantum statistical description, effective electron-ion potentials are used which account for both the screening due to the dense plasma and the inner ionic structure. Within the quantum mechanical first Born approximation, the consideration of the ionic structure leads to a drastic increase of the IB heating rate, in particular for high nuclear charges and low ionic charge states. However, for the parameters relevant in experiments, the applicability of the first Born approximation is questionable. Therefore, quantum mechanical calculations going beyond the first-order perturbation theory are performed. In addition, the IB heating rate is investigated with different classical methods. These are based either on transport cross sections for elastic electron-ion scattering or on classical simulations of inelastic scattering processes. Also within the classical approaches, the consideration of the ionic structure leads to an increase of the heating rate. However, this increase is shown to be only moderate. In a further part, the thesis focuses on the question how the dynamics of the laser-cluster interaction is influenced by the consideration of excited states. This is explored exemplarily for argon clusters excited by single or double laser pulses. The consideration of excitation processes in the nanoplasma leads to a decrease of the electron temperature and to an increase of the density of free electrons. Moreover, it is shown that the consideration of excitation processes results in an essential acceleration of the ionization dynamics. As a consequence, the mean ionic charge state in the plasma as well as the number of highly charged ions is significantly increased. For the population of ground states and excited states within an ionic charge state Z, collisional deexcitation processes play an important role. By means of an analytical relation between excitation and deexcitation cross sections, the rates for the respective processes in the presence of the laser field are calculated. The role of deexcitation processes is studied in detail, showing that the inclusion of these processes is essential for the correct theoretical description of the photon emission from laser-excited clusters. Based on these results, the photon yield is calculated for selected radiative transitions resulting from highly charged argon ions in the UV and X-ray regime.
During the past decade, various physical properties of the Yukawa ball, like structure and energy states, were unraveled using experiments. However, the dynamical features served further attention. Therefore, the main aim of my thesis was to investigate and understand how a finite system-represented by Yukawa clusters-evolves from a solid, crystalline structure to a liquid-like system, how it behaves in this phase and in what manner the reordering back into the solid state can be described. As a method of choice to reach this goal, laser heating has been proven successful. Moreover, the special importance of wakefields for dust clusters confined at low neutral gas pressure was addressed. Melting of finite dust clouds can be induced in two ways, either by altering the properties of the ambient plasma or by laser heating. The latter was shown to be a generic melting scenario, allowing to estimate a critical coupling parameter at the melting point. Moreover, the melting transition of finite 3D dust systems was found to be a two-step process where angular order is lost before the radial order starts to diminish at higher energies. Next, the mode dynamics of finite 3D dust ensembles in the solid and the liquid phase was studied. Crystal and fluid modes revealed the main spectral properties of the system. The normal modes are mainly suited to describe crystalline states. Fluid modes were excited naturally and via laser heating, with excitation frequencies almost independent of the coupling parameter in the solid and the liquid-like regime. Tuning the plasma parameters can be used to vary the particle-particle interaction via the ion focus. Both methods, even though assuming equilibrium situations, allowed to hint at these wakefields. The corresponding peaks in the fluid and normal mode spectra were no eigenmodes, confirming the nonequilibrium character of the ion focusing effect. First steps to extend the normal mode theory to achieve the dynamics of wake-affected nonequilibrium dust clusters were presented. Statistical quantities were obtained evaluating long-run experiments and transport coeffcients for finite dust systems were calculated via the instantaneous normal mode technique. Diffusion was found considerably higher for 3D than for 2D dust clusters. Using the configurational entropy, we have shown that in 2D and 3D disorder increases with increasing size of the system, in agreement with simulations. The temperature dependence of the configurational entropy differs for 2D and 3D dust clouds, with a threshold behavior found for finite 2D ensembles only. Finally, using instantaneous normal modes to reveal the total fraction of unstable modes, the predictive connection of Keyes (Phys Rev E 62, p7905, 2000), between transport and disorder was tested and verified for 2D, but not for 3D clusters. The reason for this has to be left open. Finally, laser-mediated recrystallization processes of finite 3D dust clouds were investigated. First, the temporal evolution of the Coulomb coupling parameter was traced during heating and recrystallization. A cooling rate has been determined from the initial phase of recrystallization. This cooling rate is lower than damping by the neutral gas, in agreement with simulations. We have observed a large fraction of metastable states for the final cluster configurations. Further, we have revealed that the time scale for the correlation buildup in the finite 3D ensemble was on even slower scales than cooling. Thus, different time scales can be attributed to the fast emergence of the shells and to the slower individual ordering within the shells.
Im Fokus dieser Arbeit standen die Wechselwirkungen zwischen nicht-thermischem Atmosphärendruck-Plasma und in-vitro kultivierten Keratinozyten (HaCaT-Keratinozyten) und Melanomzellen (MV3). Für die Untersuchungen wurden drei Plasmaquellen unterschiedlicher Bauart genutzt; ein Plasmajet (kINPen 09) und zwei Quellen, die das Plasma mittels der dielektrisch behinderten Entladung (Oberflächen-DBE, Volumen-DBE) generieren. Um grundlegende Effekte von Plasma auf Zellen analysieren zu können, wurde zunächst der Einfluss von physikalischem Plasma auf die Vitalität; die DNA und die Induktion von ROS untersucht. Folgende Methoden wurden verwendet: - Vitalität: - Neutralrotassay, Zellzählung (Zellzahl, Zellintegrität) - BrdU-Assay (Proliferation) - Annexin V und Propidiumiodid- Färbung, Durchflusszytometrie (Induktion von Apoptose) - DNA: - Alkalischer Comet Assay (Detektion von DNA-Schäden) - DNA-Färbung mit Propidiumiodid, Durchflusszytometrie (Zellzyklusanalyse) - ROS: - H2DCFDA-Assay, Durchflusszytometrie (Bestimmung der ROS-positiven Zellen) Neben den Folgen die die Plasmaquellen induzieren wurde weiterhin untersucht, welchen Einfluss das Behandlungsregime (direkt, indirekt, direkt mit Mediumwechsel), das Prozessgas (Argon, Luft) und die zellumgebenden Flüssigkeiten (Zellkulturmedien: IMDM, RPMI; Pufferlösungen: HBSS, PBS) auf das Ausmaß der Plasma-Zell-Effekte hatten. Die Verwendung aller Plasmaquellen führte in HaCaT-Keratinozyten und Melanomzellen (MV3) zu Behandlungszeit-abhängigen Effekten: - Verlust an vitalen Zellen und verminderte Proliferationsfähigkeit - Induktion von Apoptose nur nach den längsten Plasmabehandlungszeiten - DNA-Schäden 1 h nach Plasmabehandlung, nach 24 h deutlich weniger bzw. nicht mehr nachweisbar, Hinweise für DNA-Reparatur vorhanden - Zellzyklusarrest in der G2/M-Phase zulasten der G1-Phase 24 h nach Plasmabehandlung - Anstieg der ROS-positiven Zellen 1 h und 24 h nach Plasmabehandlung Es wurde gezeigt, dass in RPMI-Medium kultivierte Zellen sensitiver, in Form von verminderter Vitalität und vermehrten DNA-Schäden, reagierten als in IMDM-Medium gehaltene Zellen. Aber auch während der Plasmabehandlung in Pufferlösungen (HBSS, PBS) gehaltene HaCaT-Zellen wiesen DNA-Schäden auf. Die direkte und indirekte Plasmabehandlung führte zu nahezu gleichen Ergebnissen. Ein Wechsel des Zellkulturmediums direkt nach der Plasmabehandlung schwächte alle gemessenen Effekte ab. Daraus kann geschlussfolgert werden, dass neben der Art der Flüssigkeit und Behandlungszeit auch der Inkubationszeitraum der Zellen mit der in Plasma in Kontakt gekommenen Flüssigkeit von essentieller Bedeutung ist. Die durch Plasma induzierten reaktiven Spezies gelangen in die Flüssigkeit und interagieren mit den Wassermolekülen und den organischen Molekülen der Zellkulturmedien, welche langlebige Radikale (z.B. H2O2) bilden, die dann ihrerseits mit zellulären Molekülen reagieren. Die anderen Plasmakomponenten wie UV-Licht und elektrische bzw. magnetische Feldern scheinen nur eine untergeordnete Rolle in der Plasma-Zell-Interaktion zu spielen, da diese nur bei der direkten Behandlung mit den Zellen in Berührung kommen und die starken Auswirkungen nach der indirekten Behandlung nicht verursachen können. Die in diesen Untersuchungen verwendete Oberflächen-DBE konnte mit Luft oder mit Argon als Prozessgas betrieben werden. Wurde Argon als Prozessgas genutzt, kam es zu milderen Auswirkungen im Vergleich zur Plasmabehandlung im Luftmodus. Mit Luft generiertes Plasma weist neben ROS auch RNS in der Gasphase auf, letztere lassen sich im Argon-Plasma nicht nachweisen und stehen für Plasma-Zell-Interaktionen nicht zur Verfügung. Zusätzlich zu den humanen Keratinozyten wurden auch humane Melanomzellen mit Plasma (Oberflächen-DBE/Luft) behandelt. Im Vergleich zu den HaCaT-Zellen sind bei den MV3-Zellen geringere Behandlungszeiten nötig, um biologisch gleichwertige Effekte zu bewirken. Die hier verwendeten Testmethoden eignen sich für die biologische Charakterisierung von neuen Plasmaquellen bzw. für die Analyse von Plasma-Zell-Wechselwirkungen weiterer Zelllinien. Tiefergehende Untersuchungen, z.B. bezüglich der genaueren Spezifizierung der durch Plasma hervorgerufenen oxidativen DNA-Schäden und den daraus resultierenden Reparaturmechanismen, sollten folgen.
In dieser Arbeit wurde die Wirksamkeit der Antiseptika Chlorhexidindigluconat CHX 0,0001 % u. 0,00000625 %), Polihexamethylenbiguanid (PHMB 0,0001 % u. 0,000025 %) und Octenidinhydrochlorid (OCT 0,0002 % u. 0,00005 %) mit gewebekompatiblen Atmosphärendruckplasmen (TTP) mit dem Edelgas Argon als Trägergas mit und ohne Zumischung von 1% Sauerstoff, generiert mit dem kINPen09 und einer Hohlelektroden-Dielectric-Barrier Discharge Plasmaquelle (HDBD) sowie der alleinigen Gasbehandlung (Trägergas ohne Plasmagenerierung) in Bezug auf die Vermehrungshemmung bzw. Eradikation von C. albicans ATCC 10231, C. albicans SC 5314, P. aeruginosa ATCC 9027, P. aeruginosa SG 81, S. epidermidis ATCC 12228, S. epidermidis RP 62A, S. mutans DSM 20523 und S. sanguinis DSM 20068 untersucht. Die Antiseptika wirkten über den gesamten Untersuchungszeitraum von 32 h auf die Mikroorganismen ein, die TTP-Behandlungen nur 60 s. Die Vermehrung der Mikroorganismen wurde alle 30 min anhand der optischen Dichte der Testkulturen gemessen und die Fläche unter dem resultierenden Graphen (Area under the curve, AUC) charakterisiert. Bei C. albicans ATCC 10231 und SC 5314 wurde die Vermehrung vollständig von OCT 0,0002 % und der Plasmabehandlung mit HDBD mit Sauerstoffzuführung gehemmt. Die HDBD-und kINPen09- Behandlungen ohne Sauerstoffzufuhr waren beim ATCC-Stamm nur unwesentlich weniger effektiv. Die restlichen Antiseptika zeigten nur eine geringe Wirkung. Bei der Behandlung von P. aeruginosa SG 81 kam es weder durch die verwendeten Antiseptika noch durch das Plasma zu einer vollständigen Vermehrungshemmung. Insgesamt stellten sich hier die Plasmabehandlungen als deutlich effektiver heraus als die Behandlungen mit den Antiseptika. Auch bei P. aeruginosa ATCC 9027 zeigte die Behandlung mit den Antiseptika einen geringeren Effekt. Im Ganzen reagierten die gramnegativen P. aeruginosa in diesen Versuchen am wenigsten empfindlich auf die antiseptischen Behandlungen. Bei der Behandlung von S. epidermidis RP 62A bewirkten die Antiseptika PHMB 0,0001 % und OCT 0,0002 % eine vollständige Vermehrungshemmung. Die Argongaskontrolle und die Plasmabehandlung mit dem kINPen09 waren ebenso wie die Behandlung mit CHX 0,0001 % etwas weniger wirksam. Beim nicht biofilmbildenden ATCC 12228 Stamm von S. epidermidis, der nicht mit Plasma behandelt wurde, führte nur OCT 0,0002 % zu einer vollständigen Vermehrungshemmung. Bei S. mutans DSM 20523 konnte keine der untersuchten antiseptischen Behandlungen zu einer vollständigen Vermehrungshemmung führen. Am effektivsten stellten sich die Behandlungen mit OCT, PHMB und die Plasmaanwendung mit dem kINPen09 ohne und mit 1 % Sauerstoffbeimischung heraus. Die Behandlung von S. sanguinis DSM 20068 wurde ausschließlich mit Plasma bzw. deren Gaskontrollen durchgeführt. Hier waren die Plasmabehandlungen mit dem kINPen09 und deren Gaskontrollen den HDBD-Behandlungen überlegen. Von allen getesteten Antiseptika stellte sich Octenidin 0,0002 % als das am breitesten wirksame und effektivste Antiseptikum heraus. Bei der Behandlung der Candida- und S. epidermidis-Stämme führte dies zu einer vollständigen Hemmung der Proliferation bis zum Ende des Beobachtungszeitraums von 32 h. CHX 0,0001 % und PHMB 0,0001 % unterschieden sich bis auf die Behandlung von S. epidermidis RP 62A und S. mutans DSM 20523 mit der Überlegenheit für PHMB 0,0001 % nicht in ihrer Wirksamkeit. Die Plasmabehandlungen von 60 s waren mit Ausnahme von S. epidermidis den über den gesamten Untersuchungszeitraum einwirkenden Antiseptika ebenbürtig oder signifikant überlegen. Die Behandlung mit TTP könnte damit eine wirksame Alternative oder Ergänzung zu den herkömmlichen Antiseptika darstellen, um z.B. die Vermehrung von Mikroorganismen in einer infizierten Wunde zu hemmen und somit die Immunabwehr zu unterstützen und Entzündungen zu verzögern oder zu verhindern.
There is a growing interest in the application of non-thermal atmospheric pressure plasma for the treatment of wounds. Due to the generation of various ROS and RNS, UV radiation and electric fields plasma is a very promising tool which can stimulate skin and immune cells. However, not much is known about the mammalian cell responses after plasma treatments on a molecular level. The present work focusses on the impact of plasma on cell signaling in the human keratinocyte cell line HaCaT by using the methods DNA microarray, qPCR, ELISA and flow cytometry. Here, cell signaling mediators such as cytokines and growth factors which could promote wound healing by enhancing angiogenesis, reepithelization, migration and proliferation were of major interest. Additionally, the crosstalk between keratinocytes and monocytes was studied using a co-culture. For the first time extensive investigations on the impact of plasma on cell signaling in human keratinocytes were conducted. The most prominent cytokines and growth factors which were regulated by plasma at gene and protein level were VEGF-A, GM-CSF, HB-EGF, IL-8, and IL-6. The latter was not activated due to the JAK/STAT-pathway but probably by a combined activation of MAPK- and PI3K/Akt-pathways. By the use of conditioned medium it was found out that ROS and RNS generated directly after plasma treatment induced larger effects on cell signaling in keratinocytes than the subsequently secreted growth factors and cytokines. Furthermore, monocytes and keratinocytes hardly altered their secretion profiles in co-culture. From these results it is deduced that the plasma generated reactive species are the main actors during cell signaling. In order to differentiate the impact of ROS and RNS on the cellular response the ambience of the plasma effluent was controlled, varying the ambient gas composition from pure nitrogen to pure oxygen. Thereby a first step towards the attribution of the cellular response to specific plasma generated reactive species was achieved. While IL-6 expression correlated with ROS generated by the plasma source, the cell signaling mediators VEGF-A, GM-CSF and HB-EGF were significantly changed by RONS. Above all hydrogen peroxide was found to play a dominant role for observed cell responses. In summary, plasma activates wound healing related cell signaling mediators as cytokines and growth factors in keratinocytes. It was also shown that the generated reactive species mainly induced cell signaling. For the first time cell responses can be correlated to ROS and RONS in plasma treated cells. These results underline the potential of non-thermal atmospheric pressure plasma sources for their applications in wound treatment.
The confinement of energy has always been a challenge in magnetic confinement fusion devices. Due to their toroidal shape there exist regions of high and low magnetic field, so that the particles are divided into two classes - trapped ones that are periodically reflected in regions of high magnetic field with a characteristic frequency, and passing particles, whose parallel velocity is high enough that they largely follow a magnetic field line around the torus without being reflected. The radial drift that a particle experiences due to the field inhomogeneity depends strongly on its position, and the net drift therefore depends on the path taken by the particle. While the radial drift is close to zero for passing particles, trapped particles experience a finite radial net drift and are therefore lost in classical stellarators. These losses are described by the so-called neoclassical transport theory. Recent optimised stellarator geometries, however, in which the trapped particles precess around the torus poloidally and do not experience any net drift, promise to reduce the neoclassical transport down to the level of tokamaks. In these optimised stellarators, the neoclassical transport becomes small enough so that turbulent transport may limit the confinement instead. The turbulence is driven by small-scale-instabilities, which tap the free energy of density or temperature gradients in the plasma. Some of these instabilities are driven by the trapped particles and therefore depend strongly on the magnetic geometry, so the question arises how the optimisation affects the stability. In this thesis, collisionless electrostatic microinstabilities are studied both analytically and numerically. Magnetic configurations where the action integral of trapped-particle bounce motion, J, only depends on the radial position in the plasma and where its maximum is in the plasma centre, so-called maximum-J configurations, are of special interest. This condition can be achieved approximately in quasi-isodynamic stellarators, for example Wendelstein 7-X. In such configurations the precessional drift of the trapped particles is in the opposite direction from the direction of propagation of drift waves. Instabilities that are driven by the trapped particles usually rely on a resonance between these two frequencies. Here it is shown analytically by analysing the electrostatic energy transfer between the particles and the instability that, thanks to the absence of the resonance, a particle species draws energy from the mode if the frequency of the mode is well below the charateristic bounce frequency. Due to the low electron mass and the fast bounce motion, electrons are almost always found to be stabilising. Most of the trapped-particle instabilities are therefore predicted to be absent in maximum- J configurations in large parts of parameter space. Analytical theory thus predicts enhanced linear stability of trapped-particle modes in quasi-isodynamic stellarators compared with tokamaks. Moreover, since the electrons are expected to be stabilising, or at least less destabilising, for all instabilities whose frequency lies below the trapped-electron bounce frequency, other modes might benefit from the enhanced stability as well. In reality, however, stellarators are never perfectly quasi-isodynamic, and the question thus arises whether they still benefit from enhanced stability. Here the stability properties of Wendelstein 7-X and a more quasi-isodynamic configuration, QIPC, are investigated numerically and compared with another, non-quasiisodynamic stellarator, the National Compact Stellarator Experiment (NCSX) and a typical tokamak. In gyrokinetic simulations, performed with the gyrokinetic code GENE in the electrostatic and collisionless approximation, several microinstabilities, driven by the density as well as both ion and electron temperature gradients, are studied. Wendelstein 7-X and QIPC exhibit significantly reduced growth rates for all simulations that include kinetic electrons, and the latter are indeed found to be stabilising when the electrostatic energy transfer is analysed. In contrast, if only the ions are treated kinetically but the electrons are taken to be in thermodynamic equilibrium, no such stabilising effect is observed. These results suggest that imperfectly optimised stellarators can retain most of the stabilising properties predicted for perfect maximum-J configurations. Quasi-isodynamic stellarators, in addition to having reduced neoclassical transport, might therefore also show reduced turbulent transport, at least in certain regions of parameter space.
Im Rahmen der vorliegenden Arbeit wurden erstmalig systematische Untersuchungen zum Thema „Plasma-Flüssigkeits-Wechselwirkungen“ dargestellt. Es gelang mit Hilfe einer geeigneten kalten Atmosphärendruckplasmaquelle in Form einer dielektrisch behinderten Oberflächenentladung (DBE) ein Plasma in verschiedenen Arbeitsgasen zu zünden und Flüssigkeiten ohne direkten Plasmakontakt zu behandeln. Um einen Einblick in die komplexen Mechanismen zu bekommen, wurde im analytischen Teil dieser Arbeit das Plasma mittels OES untersucht, die angrenzende Gas-Phase mittels FT-IR-Spektroskopie und MS, und anschließend die Flüssigkeit unter Nutzung photometrischer Methoden und pH-Wert-Messungen. Auf der Basis dieser Untersuchungen folgten theoretische Ausführungen zu möglichen Wechselwirkungen der detektierten Komponenten mit der Flüssigkeit. Theoretisch entstehen bei der Luftplasmabehandlung von Wasser, über Zwischenprodukte (ROS und RNS) wie z. B. HO•, HOO•, NO•, NO2•, schlussendlich H+, NO3-, NO2- und H2O2. Bei der Argon- und Argon-Sauerstoff-Plasmabehandlung von Wasser dürften aufgrund des Stickstoffmangels nur ROS entstehen, die in der Entstehung von H+ und H2O2 enden. Diese Hypothesen zur Bildung der Spezies NO3-, NO2- und H2O2, sowie die Ansäuerung der Flüssigkeit wurden mittels photometrischer Methoden und pH-Wert-Messungen überprüft und bestätigt. Im anschließenden biologischen Teil der vorliegenden Arbeit wurde der Einfluss der Plasmabehandlungen in den verschiedenen Arbeitsgasen auf in physiologischer NaCl-Lösung und PBS suspendierte Mikroorganismen (E. coli, S. aureus und B. atrophaeus Sporen) untersucht. In ungepuffertem Medium wurden die vegetativen Mikroorganismen innerhalb weniger Minuten Plasmabehandlung inaktiviert. In PBS hingegen wurden längere Behandlungszeiten benötigt. Das Plasma hatte auf die suspendierten Sporen wie erwartet kaum eine inaktivierende Wirkung. Die zwei vermutlichen Hauptwege laufen einerseits über reaktive Stickstoffspezies (RNS) und andererseits über reaktive Sauerstoffspezies (ROS). RNS können in Wechselwirkung mit Wasser über diverse zelltoxische Zwischenprodukte wie z. B. NO•, NO2•, N2O3, ONOOH, ONOO- zu NO3- und NO2- umgesetzt werden. ROS in Interaktion mit Wasser resultieren in Bildung von H+ und H2O2. Auch hier wird angenommen, dass eine Vielzahl an antimikrobiellen Komponenten entsteht, z. B. HO•, HOO•, O2•-. Es gibt folglich sehr viele Reaktionen und Interaktionen zwischen plasmagenerierten reaktiven Spezies und Wasser, welche in zelltoxischen Komponenten enden und die inaktivierende Wirkung des Plasmas auf suspendierte Mikroorganismen erklären. Um die Interaktionen zwischen den Phasen Plasma-Gas-Flüssigkeit besser zu verstehen und Hypothesen zu prüfen, wurden einerseits die Mikroorganismen-Suspensionen und destilliertes Wasser nur mit plasmabehandeltem Gas behandelt und andererseits die Mikroorganismen plasmabehandelter Flüssigkeit ausgesetzt. Die Untersuchungen zeigten deutlich, dass die plasmainitiierte Chemie und damit die biologischen Effekte des Plasmas auf das Gas bzw. in Flüssigkeit übertragen werden. Folglich werden biologische Effekte des Plasmas über die Gas- und Flüssigkeits-Phase vermittelt und Plasma-Flüssigkeits-Wechselwirkungen müssen immer im zusammenhängenden chemischen System Plasma-Gas-Flüssigkeit(-Zelle) betrachtet werden. Weiterhin wurden chemische und mikrobiologische Effekte durch den Einfluss von gasförmigem NO• und O3 auf Wasser bzw. suspendierte Mikroorganismen untersucht und mit der Luftplasmabehandlung verglichen. Hierbei zeigten beide Begasung deutlich geringere inaktivierende Effekte als die Luftplasmabehandlung. Die Begasung von Mikroorganismen mit NO• und O3 und die Analytik von begastem Wasser geben einen detaillierten Einblick in die Chemie und Mechanismen der RNS und ROS. Die Behandlung mit der dielektrisch behinderten Oberflächenentladung in Luft vereint diese zwei Hauptwege über RNS und ROS und resultierte somit in effektiveren antimikrobiellen Wirkungen. Durch die Experimente der vorliegenden Arbeit wurde ein geeignetes biologisches Modell gefunden und validiert, um den Einfluss von Plasma auf lebende Zellen zu untersuchen und Mechanismen von Plasmabehandlungen aufzudecken. Anhand des Modells „Mikroorganismen-Suspension“ konnte gezeigt werden, dass die Gas-Phase (Behandlungen mit DBE-Abgas) und die extrazelluläre Flüssigkeit (Behandlungen mit plasmabehandelter Flüssigkeit) eine bedeutende Rolle bei der Vermittlung der Plasmaeffekte spielen. Die Spezies aus dem Plasma gelangten über die Gas-Phase durch Diffusion/Penetration/ Interaktion in die Flüssigkeits-Phase, reagierten teilweise zu anderen reaktiven Spezies weiter und erreichten so die Zellen. Die verschiedenen analytischen Methoden und anschließende theoretische Betrachtungen der Phasen Plasma-Gas-Flüssigkeit gaben einen detaillierten Einblick in die chemischen Mechanismen von Plasma-Flüssigkeits-Wechselwirkungen und zeigten biologisch wirksame Komponenten auf.
The concept of the electron surface layer introduced in this thesis provides a framework for the description of the microphysics of the surplus electrons immediately at the wall and thereby complements the modelling of the plasma sheath. In this work we have considered from a surface physics perspective the distribution and build-up of an electron adsorbate on the wall as well as the effect of the negative charge on the scattering of light by a spherical particle immersed in a plasma. In our electron surface layer model we treat the wall-bound electrons as a wall-thermalised electron distribution minimising the grand canonical potential and satisfying Poissons equation. The boundary between the electron surface layer and the plasma sheath is determined by a force balance between the attractive image potential and the repulsive sheath potential and lies in front of the crystallographic interface. Depending on the electron affinity x, that is the offset of the conduction band minimum to the potential in front of the surface, two scenarios for the wall-bound electrons are realised. For x<0 electrons do not penetrate into the solid but are trapped in the image states in front of the surface where they form a quasi two-dimensional electron gas. For x>0 electrons penetrate into the conduction band where they form an extended space charge. These different scenarios are also reflected in the electron kinetics at the wall which control the sticking coefficient and the desorption time. If x<0 electrons from the plasma cannot penetrate into the solid. They are trapped in the image states in front of the surface. The transitions between unbound and bound states are due to surface vibrations. Trapping of electrons is mediated by one-phonon transitions and takes place in the upper bound states. Owing to the large binding energy of the lowest bound state transitions from the upper bound states to the lowest bound state are due to multi-phonon processes. For low surface temperatures relaxation to the lowest bound state takes place while for higher temperature a relaxation bottleneck emerges. Desorption occurs in cascades for systems without relaxation bottleneck and as a one-way process in systems with a relaxation bottleneck. From the perspective of plasma physics the most important result is that the sticking coefficient for electrons is relatively small, typically on the order of 0.001. For x>0 electron physisorption takes place in the conduction band. For this case sticking coefficients and desorption times have not been calculated yet but in view of the more efficient scattering with bulk phonons, responsible for electron energy relaxation in this case, we expect them to be larger than for the case of x<0. Finally, we have studied the effects of surplus electrons on the scattering of light by a spherical particle. For x<0 the electrons form a spherical electron gas around the particle and their electrical conductivity modifies the boundary condition for the magnetic field. For x>0 the electrons in the bulk of the particle modify the refractive index through their bulk electrical conductivity. In both cases the conductivity is limited by scattering with surface or bulk phonons. Surplus electrons lead to an increase of absorption at low frequencies and, most notably, to a blue-shift of an extinction resonance in the infrared. This shift is proportional to the charge and is strongest for submicron-sized particles. The particle charge is also revealed in a blue-shift of the rapid variation of one of the two polarisation angles of the reflected light. From our work we conclude that the electron affinity is an important parameter of the surface which should affect the charge distribution as well as the charge-up. Therefore, we encourage experimentalists to study the charging of surfaces or dust particles as a function of x. Interesting in this respect is also if or under what conditions the electron affinity of a surface exposed to a plasma remains stable. Moreover, we suggest to use the charge signatures in Mie scattering to measure the particle charge optically. This would allow a charge measurement independent of the plasma parameters and could be applied to nano-dust where conventional methods cannot be applied.
In this work, various aspects of fundamental physics and chemistry of molecular gas discharges are presented with emphasis on the interaction between species, activated by low-pressure plasmas, and surfaces. As already known, synergistic effects of multiple plasma-generated species are responsible for surface modification. However, due to the large number of internal parameters of a discharge and the complex plasma processes the identification of correlations between plasma characteristics and their effects on surfaces are complicated. Therefore, the aim of this thesis is to improve the understanding of several phenomena associated with plasma–surface interactions by measuring or calculating fundamental kinetic, transport or spectroscopic data needed to interpret measurements and hereby, to support some future applications of plasmas.
Perspektiven und Risiken des Einsatzes eines körperwarmen elektrischen Plasmas in der Medizin
(2011)
Durch die vorgestellten Studien konnte gezeigt werden, dass Temperatureffekte und UV-Strahlung, die bei der Plasma-Gewebe-Wechselwirkung entstehen, keine Gefährdung für den Menschen darstellen. Die hohe antiseptische Wirkung des Plasmas ist offensichtlich auf die Bildung großer Mengen freier Radikale speziell an der Hautoberfläche, aber auch in den Haarfollikeln zurückzuführen. Die Tatsache, dass das Plasma in die Haarfollikel eindringen kann, stellt einen deutlichen Vorteil gegenüber der Anwendung flüssiger Antiseptika dar. Um jedoch eine effektive Antiseptik der Hautoberfläche zu erreichen, ist es notwendig, Plasma-Jet-Systeme mit einem Durchmesser des Plasmastrahls von ≥ 5 mm zu entwickeln. In diesem Fall ist zu erwarten, dass die Plasmabehandlung mindestens ähnliche Ergebnisse wie die Behandlung mit Octenisept® aufweist. Es ist wahrscheinlich, dass Temperatureffekte, UV-Strahlung und Radikalbildung Synergieeffekte in der menschlichen Haut bewirken, die die antiseptische Wirkung der freien Radikale als Einzelkomponente übersteigen. Damit kommt der Plasmatechnologie in Zukunft eine besondere Bedeutung bei der Wundbehandlung zu. Darüber hinaus konnte gezeigt werden, dass die Plasmabehandlung die Penetration von Partikeln und Agentien stimuliert. Damit eröffnen sich neue Möglichkeiten für eine Plasmaanwendung im Bereich der Wirkstoffzufuhr in und durch die Haut. Inwieweit diese Wirkstoffe vor oder nach der Plasmabehandlung auf die Hautoberfläche aufgetragen werden müssen, ist Zielsetzung weiterer Untersuchungen. Generell kann festgestellt werden, dass es sich bei TTP um eine neue Technologie handelt, die ein hohes Potenzial für den klinischen Einsatz aufweist. Es ist zu erwarten, dass die Anwendung von TTP im medizinischen und biotechnischen Bereich in den nächsten Jahren stark zunehmen wird. Mit der vorliegenden Arbeit wurde eine wichtige Grundlage zur Risikobewertung der Anwendung von TTP in der Medizin geschaffen und ein Beitrag zur Klärung des Wirkungsmechanismus von Plasmen im Gewebe geleistet. Darüber hinaus konnte ein neues Anwendungsgebiet der Plasmabehandlung in Form der Stimulation der Penetration von topisch applizierten Substanzen aufgezeigt werden.
Plasmapolymerisation mit einem Atmosphärendruck-Mikroplasma-Jet zur Bildung funktioneller Schichten
(2012)
In Rahmen dieser Arbeit wurde die Plasmapolymerisation von aminogruppenhaltigen und perfluorierten Kohlenwasserstoffen mit einem Atmosphärendruck Mikroplasma Jet untersucht, mit dem Ziel einer erstmaligen erfolgreichen Abscheidung von Teflon-artigen und aminogruppenhaltigen Schichten. Hierzu wurde ein Versuchsaufbau zur Schichtabscheidung mit einem Mikroplasma-Jet bei Atmosphärendruckbedingungen konzipiert und aufgebaut. Dieser besteht im Wesentlichen aus dem Plasma-Jet und der ihn umgebenden Glaskuppel, welche die Erzeugung definierter Umgebungsatmosphären bei Normaldruck gestattet sowie vor eventuell entstehenden toxischen Reaktionsprodukten schützt. Als erste Aufgabe wurde die Deposition mit den aminogruppenhaltigen Präkursoren Cyclopropylamin (CPA) und Ethylendiamin (EDA) bearbeitet. Es zeigte sich, dass die Abscheidung im selbstorganisierten Jet-Modus möglich war. Die abgeschiedenen Schichten besitzen trotz eines kuppelförmigen Abscheidungsprofils eine homogene chemische Struktur mit einem Stickstoffgehalt von bis zu 20%, wie durch Profilometrie beziehungsweise XPS ermittelt wurde. Es wurden Werte von [NH2]/[C] zwischen 5,5 % und 3 % (EDA) sowie 4 % und 1 % (CPA) erreicht, abhängig von der Behandlungszeit der Substrate und der verwendeten Umgebungsatmosphäre. Die Schutzgasatmosphäre, bestehend aus einem Gemisch aus Stickstoff und Wasserstoff, welche dazu gedacht war die Bildung primärer Aminogruppen zu unterstützen, hatte einen negativen Effekt auf die Abscheidung. Im Vergleich zu einem Prozess an Luft wurde die Depositionsrate halbiert. Weiterhin konnte ein positiver Effekt auf den Anteil der Aminogruppen nur bei CPA festgestellt werden. Bezüglich der chemischen Zusammensetzung der Schichten wird ein erstes Modell der Plasmapolymerisationsreaktionen vorgestellt, welches auf dem wiederholten Vorgang der Abspaltung einer Aminogruppe und der nachfolgenden Reaktion der so entstandenen Radikale basiert. Bei der Bearbeitung der zweiten Aufgabe, der Deposition von fluorierten Plasmapolymer-Schichten, wurde ein spezielles Entladungsregime des Jets entdeckt. Die hierbei identifizierten Konditionen ermöglichten erstmalig die Abscheidung von C:F-Schichten mit einem Atmosphärendruck Jet. Hierbei wurden mit Octafluorcyclobutan (c-C4F8) als Präkursor, mit hohen Wachstumsraten (bis zu 43 nm/s mit N2-Atmosphäre) Schichten erzeugt. In diesen wurde mitttels XPS eine homogene chemische Struktur mit einem [F]/[C]-Verhältnis von 1,4 und einem sehr geringen Gehalt an Stickstoff und Sauerstoff nachgewiesen. Fits des hoch aufgelöst gemessenen C 1s Peaks zeigen einen Vernetzungsgrad von 44 % und ein [CF2]/[CF3]-Verhältnis von rund 1,8. Der statische Wasserkontaktwinkel bei diesen Schichten lag im Bereich von 100° – 135°. Die geforderte Hydrophobie der Schichten wurde damit erreicht. Luft als Umgebungsatmosphäre während des Beschichtungsprozesses führt nicht zu einem überwiegend ätzenden Plasmaprozess, reduziert jedoch die Depositionsrate um Faktor vier. Änderungen der chemischen Zusammensetzung der Schicht im Vergleich zur Schutzgasatmosphäre wurden nicht festgestellt. Die Verwendung von Octafluorpropan (C3F8) als Präkursor ergab nur ein minimales Schichtwachstum unter Schutzgas- und kein Wachstum unter Luft-Atmosphäre. Basierend auf den Beobachtungen anderer Autoren, wurde dies durch für die Plasmapolymerisation ungünstigere Fragmentierung des Präkursors erklärt. Das spezielle Entladungsregime, die eingeschnürte und lokalisierte bogenähnliche Entladung, wird als die Ausprägung einer --Modus Atmosphärendruck Entladung erklärt, bei der das Substrat als zweite geerdete Elektrode fungiert. Hierzu ist eine ausreichende Leitfähigkeit des Substrats notwendig. Anhand eines vereinfachten Ersatzschaltbildes werden die beobachteten Abhängigkeiten von Substratmaterial und Entladungsregime modelliert
Beams of ions and electrons are a source of free energy which can be transferred to waves via an instability. Beams exist in almost all plasma environments, but their instabilities are particularly important for the dynamics of space plasmas. In the absence of collisions, the instability drives waves to large amplitudes and forms nonlinear structures such as solitary waves. The electric fields in these waves can scatter particles in the background plasma, or disrupt currents. Both of these effects are important for the overall dynamics of the plasma. In this thesis, both electron and ion beam plasma instabilities have been investigated in the linear plasma device VINETA and using a Particle-in-Cell simulation. The electron beam instability has been demonstrated by previous authors to be a useful diagnostic for the plasma density. The spatial resolution of previous results was confirmed at a few millimetres, and a temporal resolution of 1ms was shown for the first time. An ion beam was generated with a double plasma discharge. Compared to space, this environment and indeed most laboratory plasmas have considerably higher collisionality and a limited spatial extent which introduces gradients in the plasma. Gradients perpendicular to the beam propagation direction are linked to a decrease of both the wavelength and amplitude of the instability. It was observed in both experiment and simulation that gradients in sheaths at the boundaries of the plasma not only affect the time averaged plasma parameters, but also excite instabilities. Fluctuations within the sheath spread the beam in velocity space, effectively increasing its temperature. Warmer beams require a higher drift velocity to excite an instability. This was also confirmed by experimental and numerical results. Collisions are shown to be the dominant damping force for the electron beam instability. For ions, collisions play an important role in the simulation, but appear to be overshadowed by Landau damping from impurities in the experiment. When boundary conditions are removed from the simulation, wave amplitudes increase and nonlinear effects become important. Saturation by particle trapping and coalescence of phase space holes is observed, which could eventually lead to the solitary waves as they are observed in space plasmas.
Electromagnetic Drift Waves
(2010)
In the rf-plasma of the linear magnetized VINETA experiment, different types of low-frequency waves are observed. The emphasis in this work is on the interaction mechanism between drift waves on the one and kinetic Alfven waves on the other hand. In the peaked density profile of the plasma column drift waves occur as modulation of the plasma density. As gradient driven instability, they draw their energy from the radial density gradients. Alfven waves as magnetic field fluctuations are stable in the present configuration. They are launched by a magnetic excitation antenna. Parallel conduction currents in the plasma are common to both wave phenoma. A B-dot probe as standard diagnostic tool is used to detect the fluctuating magnetic fields of both wave types. The challenge are the small induced voltages due to the low wave frequency. The probe design with an integrated amplifier close to the probe head takes this into acount. The developed B-dot probe is mounted to different positioning systems to characterize both wave phenomena. For Alfven waves, the dispersion relation is recorded experimentally. It is found to be in good agreement with the prediction of the Hall-MHD theory with included resistive term, accounting for the cold collisional plasma. The fluctuating magnetic field pattern is recorded with azimuthal scans. The current density is obained by Amperes law. It is concentrated in helically twisted current filaments. For the unstable drift waves, similar investigations are done with simultaneously recorded density fluctuations. In the azimuthal plane, the locations of the parallel current filaments and the fluctuating density are found to be in phase, supporting the predicted drive of parallel currents by pressure gradients. A mutual influence of the two wave types is observed in an interaction experiment. Assuming parallel currents as coupling quantity, an interpretation of the experimental findings is given based on the linear theory of drift waves.
This thesis constitutes a computational study of charge and ion drag force on micron-sized dust particles immersed in rf discharges. Knowledge of dust parameters like dust charge, floating potential, shielding and ion drag force is very crucial for explaining complex laboratory dusty plasma phenomena, such as void formation in microgravity experiments and wakefield formation in the sheaths. Existing theoretical models assume standard distribution functions for plasma species and are applicable over a limited range of flow velocities and collisionality. Kinetic simulations are suitable tools for studying dust charging and drag force computation. The main aim of this thesis is to perform three dimensional simulations using a Particle-Particle-Particle-Mesh ($P^3M$) model to understand how the dust parameters vary for different positions of dust in rf discharges and how these parameters on a dust evolve in the presence of neighboring dust particles. At first, rf discharges in argon have been modelled using a three-dimensional PIC-MCC code for the discharge conditions relevant to the dusty plasma experiments. All necessary elastic and inelastic collisions have been considered. The plasma background is found collisional, charge-exchange collisions between ions and neutrals being dominant. Electron and ion distributions are non-Maxwellian. The dominant heating mechanism is Ohmic. Then, simulations have been done to compute the dust parameters for various sizes of dust located at different positions in the rf discharges. Dust charge and floating potential in the presheath are slightly larger than the values in the bulk due to the higher electron flux to the dust particle in the presheath. From presheath to the sheath the charge and floating potential values decrease due to the decrease of the electron current to the dust. A linear dependence of dust potential on dust size has been found, which results in a nonlinear dependence of the dust charge with the dust size when the particle is assumed to be a spherical capacitor. This has been verified by independently counting the charges collected by the dust. %where indeed it has been noted that the dust charge %scales nonlinearly with the dust size. The computed dust parameters are also compared with theoretical models. Simulated dust floating potentials are comparable to values obtained from Allen-Boyd-Reynolds (ABR) and Khrapak models, but much smaller than the values obtained from Orbit Motion Limited (OML) model. The dust potential distribution behaves Debye-H\"{u}ckel-like. The shielding lengths are in between ion and electron Debye lengths. % indicating shielding by both ions and electrons. Further, the orbital drag force is typically larger than the collection drag force. The total drag force for the collisional case is larger than for the collisionless case and it scales nonlinearly with the dust size. The collection drag values and size-scaling agrees with Zobnin's model. The charging and drag force computation is then extended to two and multiple static dust particles in the rf discharge to study the influence of neighboring dust particles on the dust parameters. Initially, the dust parameters on two dust particles are computed for various interparticle separation distances and for dust particles placed at different locations in the rf discharge. It is observed that for dust separations larger than the shielding length the dust parameters for the two dust particles match with the single dust particle values. As the dust separation is equal to or less than the shielding length the ion drag force increases due to the buildup of a parallel drag force component. However, the main dust properties like charge, potential, vertical component of ion drag are not affected considerably. This is attributed to the smaller collection impact parameter values compared to the dust separation. %This is because the %collection impact parameter values in the sheath and the presheath are smaller %than the smallest dust separation and in case of the dust in the bulk, the %collection impact parameter is comparable with the dust separation. Then the dust charges on multiple dust particles located at different positions in the discharge and arranged along the discharge axis are also computed. It is found that the charges of the multiple dust particles in the bulk or presheath do not differ much from the single particle values at that location. But the dust charges of multiple dust particles located in the sheath drastically differ from the single dust parameter values. Due to ion focusing from dust particles in the upper layers, the ion current increases to dust particles in the lower layers resulting in smaller charge values. This is as well the case where dust particles are vertically aligned as in the standard experiments of dusty plasmas. In conclusion, this work used a fully kinetic (PIC and MD or $P^3M$) model to study the physics of dust charging in rf plasmas. Our simulations revealed that the dust parameters vary considerably from the bulk to the sheath. The CX collisions increase flux to the dust thereby affecting the dust parameters and their scaling with dust size. Also, a dust particle affects the charging dynamics of its neighbor only when their separation is within the shielding length. In the plasma sheath, ion focussing can cause great reduction in dust charges.
The present work is the first work dealing with turbulence in the WEGA stellarator. The main object of this work is to provide a detailed characterisation of electrostatic turbulence in WEGA and to identify the underlying instability mechanism driving turbulence. The spatio-temporal structure of turbulence is studied using multiple Langmuir probes providing a sufficiently high spatial and temporal resolution. Turbulence in WEGA is dominated by drift wave dynamics. Evidence for this finding is given by several individual indicators which are typical features of drift waves. The phase shift between density and potential fluctuations is close to zero, fluctuations are mainly driven by the density gradient, and the phase velocity of turbulent structures points in the direction of the electron diamagnetic drift. The structure of turbulence is studied mainly in the plasma edge region inside the last closed flux surface. WEGA can be operated in two regimes differing in the magnetic field strength by almost one order of magnitude (57mT and 500mT, respectively). The two regimes turned out to show a strong difference in the turbulence dynamics. At 57mT large structures with a poloidal extent comparable to the machine dimensions are observed, whereas at 500mT turbulent structures are much smaller. The poloidal structure size scales nearly linearly with the inverse magnetic field strength. This scaling may be argued to be related to the drift wave dispersion scale. However, the structure size remains unchanged when the ion mass is changed by using different discharge gases. Inside the last closed flux surface the poloidal ExB drift in WEGA is negligible. The observed phase velocity is in good agreement with the electron diamagnetic drift velocity. The energy in the wavenumber-frequency spectrum is distributed in the vicinity of the drift wave dispersion relation. The three-dimensional structure is studied in detail using probes which are toroidally separated but aligned along connecting magnetic field lines. As expected for drift waves a small but finite parallel wavenumber is found. The ratio between the average parallel and perpendicular wavenumber is in the order of 10^-2. The parallel phase velocity of turbulent structures is in-between the ion sound velocity and the Alfvènvelocity. In the parallel dynamics a fundamental difference between the two operational regimes at different magnetic field strength is found. At 500mT turbulent structures can be described as an interaction of wave contributions with parallel wavefronts. At 57mT the energy in the parallel wavenumber spectrum is distributed among wavenumber components pointing both parallel and antiparallel to the magnetic field vector. In both cases turbulent structures arise preferable on the low field side of the torus. Some results on a novel field in plasma turbulence are given, i.e. the study of turbulence as a function of resonant magnetic field perturbations leading to the formation of magnetic islands. Magnetic islands in WEGA can be manipulated by external perturbation coils. A significant influence of field perturbations on the turbulence dynamics is found. A distinct local increase of the fluctuation amplitude and the associated turbulent particle flux is found in the region of magnetic islands.
Turbulenz ist allgegenwärtig in der Natur. Ein wichtiges Charakteristikum sind Fluktuationen auf einer Vielzahl von räumlichen und zeitlichen Skalen, die sowohl in neutralen Fluiden und gasförmigen Systemen, als auch in Plasmen beobachtet werden. Obwohl der elektromagnetische Charakter von Plasmen eine erhöhte Komplexität von Plasmaturbulenz bedingt, sind die grundlegenden Eigenschaften universell. In magnetisch eingeschlossenen Plasmen führen fluktuierende Plasmaparameter zu turbulentem Transport von Plasmateilchen und Energie, der die Einschlusszeit verringert und wichtige Aspekte zukünftiger Fusionskraftwerke beeinflusst. Der intermittente Charakter dieses konvektiven Teilchenflusses ist verbunden mit turbulenten Strukturen mit großen Amplituden, auch "blobs" genannt, die radial durch das Magnetfeld propagieren. Intermittente Fluktuationen im Randplasma von Experimenten mit linearer Magnetfeldgeometrie werden ebenfalls propagierenden turbulenten Strukturen zugeschrieben. Dabei ist der Mechanismus der radialen Propagation kaum verstanden. In dieser Arbeit wird die Bildung und Propagation von turbulenten Strukturen im linear magnetisierten Helikonexperiment Vineta untersucht. Durch Messungen der Fluktuationen in der azimuthalen Ebene mit multi-dimensionalen Sonden wird gezeigt, dass turbulente Strukturen in Driftwellenturbulenz im Gebiet des maximalen Dichtegradienten entstehen. Die turbulenten Strukturen propagieren hauptsächlich azimuthal in Richtung der Hintergrund ExB-Drift, aber sie besitzen auch eine starke radiale Geschwindigkeitskomponente. Die radiale Propagation wird durch das selbstkonsistente Potential der turbulenten Struktur verursacht, dass zu einem fluktuations-induzierten radialen Transport führt. Im Plasmarand werden die turbulenten Strukturen als intermittente Dichteeruptionen mit großen Amplituden beobachtet. Ein Vergleich der experimentellen Ergebnisse mit numerischen dreidimensionalen Fluid-Simulationen mit abgestimmten Geometrie- und Randbedingungen zeigt Übereinstimmung. Die Bildung der turbulenten Strukturen ist kausal mit einer quasi-kohärenten Driftmode verbunden und ihre radiale Propagation wird durch das selbstkonsistente elektrische Feld verursacht, dass aus der dreidimensionalen Dynamik resultiert. Zum Vergleich wird die Propagation von turbulenten Strukturen im Randplasma vom National Spherical Torus Experiment (NSTX) untersucht und mit theoretischen Propagationsmodellen verglichen.
The present experimental work investigates plasma turbulence in the edge region of magnetized high-temperature plasmas. A main topic is the turbulent dynamics parallel to the magnetic field, where hitherto only a small data basis existed, especially for very long scale lengths in the order of ten of meters. A second point of special interest is the coupling of the dynamics parallel and perpendicular to the magnetic field. This anisotropic turbulent dynamics is investigated by two different approaches. Firstly, spatially and temporally high-resolution measurements of fluctuating plasma parameters are investigated by means of two-point correlation analysis. Secondly, the propagation of signals externally imposed into the turbulent plasma background is studied. For both approaches, Langmuir probe arrays were utilized for diagnostic purposes. The main findings can be summarized as follows: Greatly elongated fluctuation structures exist in plasma edge turbulence. The structures are aligned along the confining magnetic field (k|| = 0). The correlation degree of fluctuations for a short connection length of 0.75m is greater than 80%. For much longer connection lengths of 23m and 66m, the correlation degree is reduced to approximately 40%. A conceptual interpretation of these observations is the coexistence of two different fluctuation components. One component has a correlation length parallel to the magnetic field below 20m and the other component a correlation length greater than 70m. Sine signals in the frequency range 1-100 kHz were injected into the turbulent plasma background. The propagation parallel and perpendicular to the magnetic field of the signals was studied. In poloidal direction, an asymmetry is observed, that can be explained by a copropagation of the signal with the background E × B-rotation of the plasma. The signal propagation parallel to the magnetic field shows no such asymmetry. As an advanced approach, spatio-temporal wave patters were injected into the edge plasma. The waves launched that way can be seen as test waves' in a turbulent background. The coupling strength of the imposed wave patterns to the background turbulence relies on the match of the imposed waves to the dynamics of turbulent structures. If the propagation direction of the imposed waves is parallel to the propagation direction of the background plasma, improved coupling is observed. This finding underlines the importance of the background plasma rotation for future attempts of controlling the plasma edge turbulence. Further optimization of frequency and wave vector of the imposed waves is probably a promising approach for achieving a significant and systematic influence of turbulence. Taking into account the present experimental state-of-the-art, for a deeper insight into the mechanism of the plasma edge turbulence of magnetized high-temperature plasmas a joint effort of numerical modeling and experimental results is a valuable approach. Such a cooperation should cover the explanation of the correlation observations as well as the experiments on signal injection into background turbulence. A quantitative comparison between the results presented in this work and a dedicated numerical drift wave simulation would be a significant step forward to a better understanding of plasma edge turbulence.
Two main aspects concerning drift wave dynamics in linear, magnetized plasma devices are addressed in the work: In part I of the thesis, drift waves are studied in a helicon plasma. The plasma parameter regime is characterized by comparably high collision frequencies and comparably high plasma-p exceeding the electron-ion mass ratio. Single Langmuir probes and a poloidal probe array are used for spatiotemporal studies of drift waves as well as for characterization of background plasma parameters. The main goals are the identification of a low-frequency instability and its major destabilization mechanisms. All experimentally observed features of the instability were found to be consistent with drift waves. A new code, based on a non-local cylindrical linear model for the drift wave dispersion, was used to gain more insight into the dominating destabilzation mechanisms, and also into dependencies of mode frequencies and growth rates on different parameters. In the experiment and in the numerical model, poloidal mode structures were found to be sheared. Part II of the thesis reports about mode-selective spatiotemporal synchronization of drift wave dynamics in a low-P plasma. Active control of the fluctuations is achieved by driving a preselected drift mode to the expense of other modes and broadband turbulence. It is demonstrated that only if a resonance between the driver signal and the drift waves in both space and time is reached, the driver has a strong influence on the drift wave dynamics. The synchronization effect is qualitatively well reproduced in a numerical simulation based on a Hasegawa-Wakatani model.