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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.
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 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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.
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.