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Institute
- Institut für Physik (18) (remove)
In this thesis we have revisited the formation of the excitonic insulator (EI), which realizes an exciton condensate. In contrast to optically created exciton condensates, the EI forms in thermal equilibrium and is solely driven by the Coulomb attraction between electrons and holes. The EI phase is anticipated to occur near the semimetal-semiconductor (SM-SC) transition at low temperatures. Depending from which side the EI is approached, it forms due to a BCS-type condensation of electron-hole pairs or a Bose-Einstein condensation (BEC) of excitons. The extended Falicov-Kimball model (EFKM) is the minimal model the EI can be described with. This model describes spinless fermions in two dispersive bands (f band and c band), that interact via a local Coulomb repulsion. The EFKM is also used to describe electronic ferroelectricity (EFE). Both phases, the EI and EFE-type ordering, are characterized by a spontaneous f-c hybridization in the EFKM. We have presented the EI phase, the EFE phase, and the orderings they compete with. Moreover, we have determined the ground-state phase diagram of the EFKM. We have focused particularly on the anticipated BCS-BEC crossover within the EI and have analyzed the formation scenarios. The exciton spectrum and the exciton density in the normal phase close to the critical temperature give information about relevant particles and therefore the nature of the transition. We have demonstrated that the whole EI is surrounded by a halo", that is, a phase composed of electrons, holes and excitons. However, on the SM side, only excitons with a finite momentum exist. These excitons appear only in a small number and barely influence the SM-EI transition. This phase transition is driven by critical electron-hole fluctuations, generated by electrons and holes at the Fermi surface. On the SC side, excitons with arbitrary momenta exist. Most notably, we have found the number of zero-momentum excitons to diverge at the SC-EI transition, signaling the BEC of these particles. Within the EI phase, there is a smooth crossover from the BCS regime to the BEC regime. One of the promising candidates to observe the EI experimentally, is the transition-metal dichalcogenide 1T-TiSe2. Strong evidences were found favoring an EI scenario of the charge-density-wave (CDW) formation in this material. However, some aspects point to a lattice instability to drive the CDW transition. We have addressed this issue by analyzing the recently discovered chiral property of the CDW in 1T-TiSe2. We have found that the EI scenario is insufficient to explain a stable, long range chiral charge ordering. Lattice degrees of freedom must be taken into account. In particular, nonlinear electron-phonon coupling and phonon-phonon interaction are crucial. By estimating appropriate model parameters for 1T-TiSe2, we have suggested a combination of excitonic and lattice instability to drive the CDW transition in this material. Experiments in 1T-TiSe2 and other materials suggest that the coupling to the lattice is non-negligible. We have extended therefore the model by an explicit exciton-phonon interaction, and have analyzed crucial effects of this interaction. While the single-particle spectrum is not modified qualitatively, the electron-hole pair spectrum changes significantly. The inclusion of the phonons lead to a massive collective mode in the ordered ground state in contrast to the case for vanishing exciton-phonon coupling, where the mode is acoustic. We have suggested that a gapless collective mode leads to off-diagonal long range order. This questions that the ground state for finite exciton-phonon coupling represents a condensate.
Magnetic reconnection is a ubiquitous phenomenon observed in a wide range of magnetized plasmas from magnetic confinement fusion devices to space plasmas in the magnetotail. The process enables the release of accumulated magnetic energy by rapid changes in magnetic topology, heating the plasma in the vicinity of the reconnection site, generating fast particles and allowing a wealth of instabilities to grow. This thesis reports on the results from a newly constructed linear, cylindrical and modular guide field reconnection experiment with highly reproducible events, VINETA.II. A detailed analysis of the reconnecting current sheet properties on a macroscopic and microscopic scale in time and space is presented. In the experiment, four parallel axial wires create a figure-eight in-plane magnetic field with an X-line along the central axis, as well as an axial inductive field that drives magnetic reconnection. Particle-in-cell simulations show that the axial current is limited by sheaths at the boundaries and that electrostatic fields along the device axis always set up in response to the induced electric field. Current sheet formation requires an additional electron current source, realized as a plasma gun, which discharges into a homogeneous background plasma created by a rf antenna. The evolution of the plasma current is found to be dominantly set by its electrical circuit. The current response to the applied electric field is mainly inductive, which in turn strongly influences the reconnection rate. The three-dimensional distribution of the current sheet is determined by the magnetic mapping of the plasma gun along the sheared magnetic field lines, as well as by radial cross-field expansion. This expansion is due to a lack of equilibrium in the in-plane force balance. Resistive diffusion of the magnetic field by E=η j is found to be by far insufficient to account for the high reconnection rate E=-dΨ/dt at the X-line, indicating the presence of large electrostatic fields which do not contribute to dissipative reconnection. High-frequency magnetic fluctuations are observed throughout the current sheet which are compared to qualitatively similar observations in the Magnetic Reconnection Experiment (MRX, Princeton). The turbulent fluctuation spectra in both experiments display a spectral kink near the lower hybrid frequency, indicating the presence of lower hybrid type instabilities. In contrast to the expected perpendicular propagation of mainly electrostatic waves, an electromagnetic wave is found in VINETA.II that propagates along the guide field and matches the whistler wave dispersion. Good correlation is observed between the local axial current density and the fluctuation amplitude across the azimuthal plane. Instabilities driven by parallel drifts can be excluded due to the large required drift velocities or low resulting phase velocities that are not observed. It is instead suggested that a perpendicular, electrostatic lower hybrid mode indeed exists that resonantly excites a parallel, electromagnetic whistler wave through linear mode conversion. The resulting fluctuations are found to be intrinsic to the localized current sheet and are independent of the slower reconnection dynamics. Their amplitude is small compared to the in-plane fields, and have a negligible contribution to anomalous resistivity through momentum transport in the present parameter 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.
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.
Ausgangspunkt aller Untersuchungen sind Langmuir-Monoschichten an der Wasser/Luftgrenzfläche. Denn mit diesen Monoschichten kann die Oberflächeladungsdichte eingestellt werden. Sie werden durch amphiphile Moleküle gebildet.Die hydrophoben Alkylketten sind zur Luftseite und die hydrophile Kopfgruppe zur Wasserseite orientiert.Die Phasen der Lipid- Monoschicht und die Belegungsdichte werden extern eingestellt. Die Lipid- Monoschicht kann je nach Anordnung der Alkylketten verschiedene unter- schiedliche Phasen zeigen. Um die adsorbierten Polyelekrolyte zu beschreiben zu können, benötigt man experimentelle Methoden, die in der Lage sind, Konformation und Be- legungsdichte von adsorbierten Polyelektrolyten an Oberflächen aufzulösen. Diese Strukturen, auf der Nanometerskala, werden mit Röntgenreflektion und Röntgendiffraktion unter streifendem Einfall untersucht.Die Strukturda- ten werden durch thermodynamische Untersuchungen ergänzt. Die Untersuchungen werden für elektrostatische Kräfte mit hoher Ampli- tude und langer Reichweite durchgeführt. Die Lösungen der Polyelektrolyte (c PSS = 0.01 mmol/L bezogen auf die Monomerkonzentration) sind so einge- stellt, dass eine fast vollständige Ladungskompensation (70-90%) stattfindet. Unter diesen Bedingungen adsorbieren PE entweder flach als 2-dimensionales Knäuel oder geordnet in einer 2-dimensionalen lamellaren Phase. Die Untersuchungen sollen herausfinden, welchen Einfluss die elektrostatische Wechselwirkung auf die Kettensteifigkeit von adsorbierten Polyelektrolyten,die durch die Persistenzlänge LP charakterisiert werden.So kann geklärt werden,ab welcher Konturlänge LK Polyelektrolyte nicht mehr stäbchenförmig sondern als 2-dimensionales Knäuel adsorbieren. Untersucht werden negativ geladene PSS (Polystyron Sulfonat) mit un- terschiedlichen Konturlängen LK.Diese adsorbieren an die positiv geladene DODA Lipid-Monoschicht (Dioctadeyldimethylammonium). Die Persistenzlänge LP für adsorbiertes PSS an DODA ist direkt aus den thermodynamischen Daten ermittelt worden. Als Funktion der Konturlänge LK wurde der Oberflächendruck π c sowie die erste Ableitung dπc /dT unter- sucht. Daraus läßt sich die Persistenzlänge des adsorbierten PSS LP ≈ 210 Å bestimmen. Die Oberflächenladungsdichte der Monoschicht wird durch die Kompression verdoppelt.Simultan wird der Abstand der Polyelektrolytketten dPE halbiert, so dass immer eine 70-90% Ladungskompensation erreicht wird. Es wird mit Röntgendiffraktion immer eine fache 2-dimensionale lamellare Phase der adsorbierten PSS Ketten detektiert.Hierbei bilden Konturlängen LK < 110 Å eine Ausnahme. Es wird keine 2-dimensionale lamellare Phase für geringe Oberflächenladungsdichte (LE Phase der Lipide) gefunden. Die Röntgenreflektion kann aber zeigen, dass PSS Ketten, unabhängig von der Konturlänge LK, immer flach an der Lipidmonoschicht adsorbieren. Wenn steife kurze Ketten (LK≤110Å<LP ) an der LC Phase der Lipid- Monoschicht adsorbieren, liegen sie aber in der 2-dimensionalen lamellare Phase. Der Übergang von der LE in die LC Phase der Lipid-Monoschichten erfolgt gleichzeitig mit dem Übergang von der ungeordneten flachen zur 2- dimensionalen lamellare Phase der adsorbierten kurzen PSS Ketten. Daher zeigt die Enthalpie ∆H des LE/LC Phasenübergangs ein Maximum bei L K =110 Å. Im nächsten Schritt wird die Elektrostatik zwischen der Lipid-Monoschicht und den Polyelektrolyte untersucht.Die maximale Oberflächenladungsdichte der Lipid-Monoschicht wird durch eine Mischung von geladenen DODA und ungeladenen DPPC (Dipalmitoylphosphatidylcholine) eingestellt. Röntgendiffraktionsmessungen zeigen bis zu einem DODA-Anteil von 75% die Ausbildung einer 2-dimensionalen lamellaren Phase an der LC Phase der Lipid-Monoschicht. Nimmt die maximale Oberflächenladungsdichte weiter ab, so wird keine Bildung der 2-dimensionalen lamellaren Phase beobachtet. Die Abnahme der maximalen Oberflächenladung führt zu einer niedrigen Belegungsdichte und so zu einem größerem Kettenabstand dPE. Die Linienladungsdichte wird durch unterschiedliches P−TrisAAx−rand−AMPS1−x auf 90% oder 50% verringert. Röntgendiffraktionsmessungen an PE mit unterschiedlichen Linienladungsdichten zeigen auch hier eine 2-dimensionale lamellare Phase. Die verringerte Linienladungsdichte erzwingt eine höhere Belegungsdichte um eine 70-90% Ladungskompensation zu erreichen. Dieses führt zu einem kleineren Kettenabstand dPE. Ein Grenzfall ist bei einer 50%-igen Linienladungsdichte zu beobachten. Dort konnte an der LC Phase der Lipid-Monoschicht keine 2-dimensionale lamellare Phase der PE beobachtet werden. Der Kettenabstand dPE ist so gering, dass er mit der Röntgendiffraktion nicht mehr aufgelöst werden kann.
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 extraction of raw materials in mining, as for example copper, generally requires a separation of the natural resources quarried. In most cases complex ores, mixtures of different minerals and gangue have to be separated in order to enable an economic processing. In particular for the extraction of sulfides, oxides, carbonates, phosphates, but also of coal, froth flotation is mainly used for this purpose, therefore it is considered as the most important separation process in raw material industries. Several billion tons of ores are processed annually. The principle of flotation is based on the surface properties of the mixtures components and the separation efficiency, which decisively determines the required amount of water and various chemicals, if nothing else, is an important criterion in mineral exploration and it also significantly influences the environmental impact of mineral processing. The aim of, this work was to investigate the influence, of, low-temperature plasmas on the mineral surface and, based on the acquired knowledge, to develop and verify strategies that would increase the efficiency of flotation processes through plasma pre-treatment of mineral mixtures. Since these studies are unprecedented, the results presented can be classified as a contribution to application-oriented basic research. Powder of the sulfide minerals, pyrite (FeS2), chalcopyrite (CuFeS2), chalcocite (Cu2S) and molybdenum sulfide (MoS2), were treated with plasmas of a radiofrequency and a microwave discharge and the resulting surface modifications were investigated by structure analysis such as X-ray photoelectron spectroscopy (XPS) and X-ray diffraction (XRD). During the plasma process, the argon/oxygen and argon/hydrogen process gas mixtures used were analyzed by mass spectrometry (MS), taking into account the quantity of gaseous reaction products released, in order to estimate the rate at which chemical reactions occur. Furthermore, Langmuir and thermal probes, as well as different methods of optical emission spectrometry (OES) were utilized, which enabled a characterization of the discharges used with regard to different plasma parameters. It has been shown that sulfur dioxide (SO2) in Ar/O2 plasmas and hydrogen sulfide (H2S) in Ar/H2 plasmas are the only reaction products which can be detected by MS during the mineral treatments. Thus, the resulting sulfur rate loss could be time-resolved determined by means of additional calibrations with calibrating gases. Especially at Ar/O2-MW plasma treatments two fundamental mechanisms of mineral modification could be separated by time. Pure plasma-surface interactions at the beginning and, additionally, thermally induced reactions in during the evolution of the treatments. Comparisons regarding the relative sulfur loss during plasma-surface interactions between the investigated minerals have shown a strong influence of the process parameters whereas, under identical conditions, CuFeS2 reacted up to eight and nineteen times faster reacted than FeS2 or Cu2S. This result represents the basis of the strategy to optimize the flotation of the minerals investigated: The selective generation of oxides on the surface of one component in a mixture of sulphide minerals. In particular, at the separation of CuFeS2/FeS2 mixtures by using the oxide collectors Flotinor Fs-2 in a micro flotation cell, a high selectivity could be achieved. The recovery of CuFeS2 amounted to 100 % while less than 10 % of FeS2 was recovered and no other modifying reagents were used. XPS and XRD analyses indicate the possibility that metal oxide are created upon the CuFeS2 surface, while the formation of iron sulfates upon the FeS2 surface prevented the oxide collector adsorption. An increased intensity of the plasma treatment leads to an increased sulphate formation also on CuFeS2, whereas the recovery, and thus the selectivity of the flotation, was reduced again. It could be shown that this effect can be utilized for the separation of, CuFeS2/MoS2 mixtures by using both, oxide and sulfide collectors, because sulfates are not formed on molybdenum sulfide during Ar/O2 plasmas treatments. By means of the plasma diagnostics used the energy input onto the substrate, the gas temperature and the degree of dissociation of molecular gases were estimated and correlations regarding the surface modification have been worked out. Thereby, the region investigated within the parameter space could be enlarged due to the use of different excitation frequencies, 13.56 MHz and 2.45 GHz, and additional insights have been provided. Further studies, beyond the scope of this work, are, nevertheless, required in order to generate a more comprehensive picture of plasma-mineral interactions and to enable an optimal application of the obtained results.
The Atomic Force Microscope (AFM) has become an important tool for probing the mechanical properties of cells and microparticles by force-indentation experiments. In this thesis optimized AFM approaches for these experiments are developed and applied to three types of living human cells in order to answer biologically relevant questions about their mechanics. These microscopic investigations are then interpreted with respect to nanoscopic and macroscopic biologic parameters, such as the function of cell surface receptors or the size of human heart ventricles. This thesis comprises two physical/technical chapters and three medical/biological chapters. The physical/technical chapters discuss the measurement process itself, aiming for its improvement with respect to a proper data analysis and contact model (for spherical cells). The medical/biological chapters investigate the elasticity of cells by the use of optimized AFM approaches, with respect to the used data analysis.
Die vorliegende Arbeit liefert Beiträge zur optischen und elektrischen Charakterisierung des dynamischen Verhaltens von Plasmaspezies in Atmosphärendruck-Plasmen insbesondere mit Hinsicht auf den Einsatz in der Plasmamedizin. Dabei wurde ein breites Spektrum verschiedener Diagnostiken angewandt, um die Zugänglichkeit zur Bestimmung weiterer Plasmaparameter an Atmosphärendruck zu prüfen. Diese Arbeit stellt eine neue Methode zur Bestimmung der Ionendichte bei Atmosphärendruck- Bedingungen vor, bei der elektrische Oszillationen ausgewertet werden, deren Ursprung ionenakustische Wellen im Plasma sind. Weiterhin wurden neben relativen optischen Messungen wie der phasenaufgelösten optischen Fotografie (PROI) und der Kreuz- Korrelations-Spektroskopie (CCS) auch absolute optische Messungen mit der interferometrischen Hakenmethode und dem Pockels-Effekt durchgeführt. Anhand von elektrischen Messungen wurde ferner gezeigt, dass mit einer Strom- und Spannungs-Charakteristik der Einfluss von Aufbauparametern, wie der Kapillarposition oder dem Gasfluss, auf das Plasma untersucht werden kann. Gegenstand der Untersuchungen waren verschiedene Plasmaquellen, die für eine Nutzung in der Plasmamedizin entwickelt wurden. Sowohl die elektrischen Messungen des Parametereinflusses als auch die Bestimmung der Ionendichte erfolgten an der selbstpulsenden transienten Funkenentladung in Argon an offener Atmosphäre. Der geringe Filamentdurchmesser und der dennoch hohe Entladungsstrom ermöglichen die Detektion der ionenakustischen Instabilität. Darüber hinaus wurde diese erratisch zündende Entladung räumlich und zeitlich aufgelöst mit der CCS spektroskopisch untersucht. Dabei wird insbesondere die Selbst-Triggerung der CCS ausgenutzt, um einen Zeitbezug trotz des großen Entladungsjitter zu erhalten. Für die PROI wurden die räumlich und zeitlich stabilen Entladungsanordnungen der Nadel-Platte-Geometrie und des Kapillarjets in Helium gewählt. Die Anordnungen wurden mit einer periodischen Sinusspannung betrieben und wiesen Entladungsspalte von d = 5 - 15 mm auf. Eine besondere Anforderung der Messung mit dem Pockels-Effekt ist zu der räumlichen und zeitlichen Stabilität eine dielektrische Gegenelektrode, welche bei der Anordnung des Kapillarjets möglich war. Bei der Anwendung der interferometrischen Hakenmethode kam neben einem Erdgas-Sauerstoff-Mischgasbrenner sowohl eine Mikrowellen-Entladung (Plexc) als auch ein MHz-Plasmajet (kINPen) zur Anwendung. Die Bedeutung der elektrischen Messungen, besonders der Strom- und Spannungscharakteristik einer Entladung, wurde an dem Parametereinfluss der Kapillarposition einer erratisch zündenden transienten Funkenentladung vorgestellt. Es konnte gezeigt werden, dass der Zeitunterschied zwischen dem Stromsignal eines Vorstreamers und der Hauptentladung durch das Einbringen einer Kapillare in den Entladungsspalt deutlich verringert wird. Insbesondere der Beitrag der lokalen elektrischen Feldstärkeerhöhung an der Kapillarkante und der Diffusionsanteil der Umgebungsluft wurden als Ursachen, durch Vergleich einer Feldsimulation mit der Beobachtung der Vorphase an der Kapillarkante in den CCS-Messungen, diskutiert. Anschließend konnte gezeigt werden, dass der Leistungseintrag in die Vorphase durch die Platzierung der Kapillare deutlich reduziert werden kann. Ein wesentliches Ergebnis dieser Arbeit ist die Beobachtung von ionenakustischen Wellen als Oszillationen im Abklingen des Stromsignals einer erratisch zündenden transienten Funkenentladung. Hierzu war es nötig, elektrische Störungen zu erkennen und zu eliminieren. Es konnte ein Erdschleifen-freier Aufbau realisiert werden. In diesem Aufbau zeigt sich, dass die Signale der ionenakustischen Welle ausschließlich in einem bestimmten Gasflussbereich beobachtet werden. Die gemessene Frequenz der Oszillationen wurde als Ionenplasmafrequenz f_{pl ,i} identifiziert und enthält daher Angaben zu den Ionendichten im Bereich von n_{Ar_2^+} = 3•10^{14} cm^{-3} bis 1•10^{12} cm^{-3}. Nach einer Abschätzung der zu erwartenden Elektronendichte, die der gemessenen Ionendichte sehr nahe kommt, wurde die Dispersionsrelation für die vorhandenen Entladungsbedingungen aufgestellt und gelöst. Dabei zeigt sich eine starke zeitliche Dämpfung über die Ionen-Neutralteilchenstöße sowie eine räumliche Verstärkung für die Ionenplasmafrequenz. Aus der Dämpfung der Oszillationsamplituden konnte die Ionen- Neutralteilchen-Stoßfrequenz nu_i = 3•10^7 Hz ermittelt werden. Weiterhin ergibt sich aus der Lösung der Dispersionsrelation ein Existenzbereich für die ionenakustischen Wellen in Abhängigkeit von der Ionendichte und der elektrischen Feldstärke.