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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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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).
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.
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.
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.
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.
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.
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 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.
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.
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.