Refine
Year of publication
Document Type
- Doctoral Thesis (27)
- Article (1)
Language
- English (28) (remove)
Has Fulltext
- yes (28)
Is part of the Bibliography
- no (28)
Keywords
- Plasma (28) (remove)
Institute
- Institut für Physik (23)
- Abteilung für Mikrobiologie und Molekularbiologie (1)
- Institut für Immunologie u. Transfusionsmedizin - Abteilung Transfusionsmedizin (1)
- Institut für Pharmazie (1)
- Interfakultäres Institut für Genetik und Funktionelle Genomforschung (MNF) (1)
- Poliklinik für Kieferorthopädie, Präventive Zahnmedizin und Kinderzahnheilkunde (1)
Publisher
- S. Karger AG (1)
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.
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.
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.
The active screen plasma nitrocarburizing (ASPNC) technology is a state-of-the-art plasma-assisted heat treatment for improving surface hardness and wear resistance of metallic workpieces based on thermochemical diffusion. In comparison to conventional plasma nitrocarburizing, the use of an active screen (AS) improves thermal homogeinity at the workload and reduces soot formation. Further it can serve as a chemical source for the plasma processes, e.g. by use of an AS made of carbon-fibre reinforced carbon. This compilation of studies investigates the plasma-chemical composition of industrial- and laboratory-scale ASPNC plasmas, predominantly using in-situ laser absorption spectroscopy with lead-salt tuneable diode lasers, external-cavity quantum cascade lasers, and a frequency comb. In this way the temperatures and concentrations of the dominant stable molecular species HCN, NH3, CH4, C2H2, and CO, as well as of less prevelant species, were recorded as functions of e.g. the pressure, the applied plasma power, the total feed gas flow and its composition. Additionally, the diagnostics were applied to a chemically similar plasma-assisted process for diamond deposition.
Resulting from this thesis are new insights into the practical application of an AS made of CFC, the plasma-chemistry involving hydrogen, nitrogen, and carbon, and the particular role of CO as an indicator for reactor contamination. The effect of the feed gas composition on the resulting nitrogen- and carbon-expanded austenite layers was proven by combination of in-situ laser absorption spectroscopy with post-treatment surface diagnostics. Furthermore this work marks the first use of frequency comb spectroscopy with sub-nominally resolved Michelson interferometry for investigation of a low-pressure molecular discharge. This way the rotational bands of multiple species were simultaneously measured, resulting in temperature information at a precision hitherto not reached in the field of nitrocarburizing plasmas.
Modern space missions depend more and more on electric propulsion devices for in-space
flights. The superior efficiency by ionizing the feedgas and propelling them using electric
fields with regard to conventional chemical thrusters makes them a great alternative. To
find optimized thruster designs is of high importance for industrial applications. Building
new prototypes is very expensive and takes a lot of time. A cheaper alternative is to rely
on computer simulations to get a deeper understanding of the underlying physics. In order
to gain a realistic simulation the whole system has to be taken into account including the
channel and the plume region. Because numerical models have to resolve the smallest time
and spatial scales, simulations take up an unfeasible amount of time. Usually a self-similarity
scaling scheme is used to greatly speed up these simulations. Until now the limits of this
method have not been thoroughly discussed. Therefore, this thesis investigates the limits
and the influence of the self-similarity scheme on simulations of ion thrusters. The aim
is to validate the self-similarity scaling and to look for application oriented tools to use
for thruster design optimization. As a test system the High-Efficiency-Multistage-Plasma
thruster (HEMP-T) is considered.
To simulate the HEMP-T a fully kinetic method is necessary. For low-temperature plasmas,
as found in the HEMP-T, the Particle-in-Cell (PIC) method has proven to be the best
choice. Unfortunately, PIC requires high spatial and temporal resolution and is hence
computationally costly. This limits the size of the devices PIC is able to simulate as well
as limiting the exploration of a wider design space of different thrusters. The whole system
is physically described using the Boltzmann and Maxwell equations. Using these system
of equations invariants can be derived. In the past, these invariants were used to derive a
self-similarity scaling law, maintaining the exact solution for the plasma volume, which is
applicable to ion thrusters and other plasmas. With the aid of the self-similarity scaling
scheme the computation cost can be reduced drastically. The drawback of the geometrical
scaling of the system is, that the plasma density and therefore the Debye length does not
scale. This expands the length at which charge separation occurs in respect to the system
size. In this thesis the limits of this scaling are investigated and the influence of the scaling
at higher scaling factors is studied. The specific HEMP-T design chosen for these studies is
the DP1.
Because the application of scaling laws is limited by the increasing influence of charge separation with increased scaling, PIC simulations still are computationally costly. Another approach to explore a wider design space is given using Multi-Objective-Design-Optimization
(MDO). MDO uses different tools to generate optimized thruster designs in a comparatively
short amount of time. This new approach is validated using the PIC method. During this
validation the drawback of the MDO surfaces. The MDO calculations are not self-consistent
and are based on empirical values of old thruster designs as input parameters, which not
necessarily match the new optimized thruster design. By simulating the optimized thruster
design with PIC and recalculate the former input parameters, a more realistic thruster design is achieved. This process can be repeated iteratively. The combination of self-consistent
PIC simulations with the performance of MDO is a great way to generate optimized thruster
designs in a comparatively short amount of time. The proof of concept of such a combination
is the pinnacle of this thesis.
In this work, studies with respect to the exhaust problem were performed
in the stellarator experiment Wendelstein 7-X with different target concepts and different magnetic field geometries. Different infrared cameras were used to study the heat flux from the plasma onto the PFC. In the first publication, the limiter set-up was used with a simpler magnetic topology in the plasma edge. The radial fall-off of the parallel heat flux for inboard limiters in W7-X shows, similar to inboard limiters in tokamaks, two different radial fall-off lengths, a short (narrow) one, characterizing the near-SOL, and a long (broad) characterizing the far-SOL. For the far-SOL, the heating power and connection length have been identified as the main scaling parameters, while for the near-SOL, the electron temperature close to the LCFS has been identified as the main scaling parameter. The two fall-off lengths differ by a factor 10, and the found scalings for both regimes differ from known models and experimental scalings in tokamaks. A turbulent-driven feature was discussed in the publication as a possible explanation for the behavior of the fall-off length in W7-X.
The gained information and data have been further used to support many
other publications, covering the symmetry of the heat loads, the
energy balance of the machine, and seeding experiments.
The heat exhaust in W7-X with an island divertor was studied in the second
and third publication. Definitions of parameters such as peaking factor and
wetted area were applied for the heterogeneous heat flux pattern on the
W7-X divertor. It was shown that the island divertor concept is capable
of spreading out the heat efficiently, resulting in large wetted areas of up to 1.5 m2. The reached values for the wetted area are comparable to the ones of the larger tokamak JET but with a much smaller ratio of wetted
area to the area of the last closed flux surface. Furthermore, a positive
scaling of the wetted area with the power in the SOL was observed. This
scaling is beneficial for future reactors but needs further investigation of the involved transport processes. The peaking factor (discussed in the second publication) describes how concentrated the heat load is within the region of the strike line. It was shown that this factor is decreasing for increasing densities without affecting the wetted area. The present work paves the way for further analysis of the transport processes of the heat flux towards the island divertor of Wendelstein 7-X.
The thyroid as the largest endocrine gland mainly produces and secretes the thyroid hormones (TH): 3,3’,5-triiodo-L-thyronine (T3) and its pro-hormone L-thyroxine (T4). Besides the impact on growth, normal development, bone marrow structure, the cardiovascular system, body weight and thermogenesis, TH play a vivid role in many metabolic regulatory mechanisms in almost all tissues. Thyroid diseases are relatively prevalent and cause, due to the resulting TH imbalances, a broad spectrum of effects. Many of them manifest in pathologically increased or decreased TH levels defined as hyperthyroidism or hypothyroidism, respectively. Routinely, determination of the thyroid state is based on the assessment of the classical markers TSH and free T4. However, this practice has several drawbacks. Moreover, elucidation of the pleiotropic effects of TH on multiple molecular pathways is mostly based on cell culture, tissue and rodent models. Analysis of animal biofluids like serum and urine using metabolomics approaches demonstrated the extensive impact of TH on other body compartments. In contrast, proteome profiling has not been exploited for the comprehensive characterization of the general metabolic effects of TH. Plasma as a large and diverse compartment of the human proteome provides a great opportunity to identify novel protein markers of thyroid function as well as to characterize metabolic effects of TH in humans.
Therefore, a study of experimental thyrotoxicosis was performed with 16 male volunteers treated with 0.25 mg/d levothyroxine (L-T4) for 8 weeks to induce a hyperthyroid state. Plasma samples were collected before the L-T4 application started, two times during the treatment and additionally two times after withdrawal. Proteome analysis revealed remarkable alterations including increased levels of two known proteins known to correlate with TH levels (sex hormone-binding globulin and cystatin C). The correlation with free T4 levels revealed 76 out of 437 detected proteins with a Pearson correlation coefficient of r ≥ |0.9|. One prominent signature included 10 coagulation cascade proteins exhibiting significantly increased plasma levels during thyrotoxicosis, thereby revealing a trend towards a hypercoagulative state in hyperthyroidism. To overcome the statistical drawbacks of the Pearson correlation analysis, additionally a mixed-effect linear regression model using serum free T4 concentrations as exposure and protein abundances as outcome while controlling for age, BMI, and batch was implemented. Application of this model resulted in the detection of 63 proteins with significant associations to free T4 levels. Besides the already mentioned augmented coagulation, a significant drop in the amounts of three apolipoproteins (ApoD, ApoB-100 and ApoC3) was observed. Furthermore, an increased abundance of proteins assigned to the complement system was detected.
Experimental studies in humans were complemented by corresponding analyses in murine models. In the current work, plasma samples of two murine studies including male C57BL/6 wildtype mice were analyzed to elucidate the impact of thyroid dysfunction on the plasma proteome. The first study was similarly designed as the human model of experimentally induced thyrotoxicosis and assigned the animals to three groups: a control group, a T4 treatment group, and a T4 recovery group, whereupon the latter first received T4 followed by a subsequent TH normalization period. A high proportion of plasma proteins exhibited significantly different protein levels during T4 application (n = 120), where 90 of these also showed a corresponding reverse trend after T4 withdrawal (T4 recovery vs. T4), thereby displaying transient alterations. The molecular pattern of hyperthyroidism in the murine model indicated, as in the human study, a pronounced decrease in apolipoproteins. However, in clear contrast to the human data, the levels of proteins related to the coagulation cascade and complement system were also transiently decreased in mice, while being increased in humans.
The second murine analysis focused on the impact of hyper- and hypothyroidism caused by T3 or T4 treatment and MMI/KClO4 application, respectively. In general, compared to the first murine study less clear alterations of protein levels were detected. Proteins related to the complement system revealed fewer changes in the T3 group and only marginal changes after T4 induction. Unexpectedly, the MMI/KClO4-induced hypothyroidism caused a reduction of the levels of several proteins assigned to the complement system, although different components and factors were affected.
Generally, rodent studies partially provided a divergent picture of TH action as compared to human studies. However, in spite of inconsistent results in studies regarding the effects of TH that are possibly due to species-specific differences, an important role of TH on several metabolic and other pathways, e.g. in the process of blood coagulation and apolipoprotein regulation, is evident. The results from both murine and human studies presented here provide novel insights into changes in the plasma proteome in the context of thyroid diseases which might contribute to a better understanding of TH action on metabolism and other pathways.
The aim of this thesis is to concentrate on the investigation of these ROS&RNS composition distribution and their production pathways in the gas phase produced by a plasma jet. By understanding the physical mechanisms behind the generation of the ROS&RNS a precise tuning and design of the composition distribution in the gas phase can be achieved. One crucial physical parameter is the dissipated power inside the plasma. Only if this parameter is known a meaningful comparison of different feed gas settings is possible. Therefore, a concept for measuring the dissipated power inside the plasma for the modified micro-scaled atmospheric pressure plasma jet( µAPPJ) is designed. Additionally, due to achievements within this thesis it is now possible to ignite a homogeneous discharge in argon and helium within the geometry of the µAPPJ. The used feed gas is a determining factor concerning the electron energy distribution function and consequently influencing the production mechanism of the ROS&RNS. First of all, the electrical characterisation of the modified µAPPJ was performed including the alpha-to-gamma transition. It is shown that the alpha-to-gamma transition power is increasing with increasing frequency. For the first time it is now feasible to investigate the influence of the dissipated power on the neutral gas temperature, the metastable atom densities and the ROS&RNS production for the modified µAPPJ with argon and helium as feed gas. Due to the possibility of changing the feed gas and controlling the dissipated power a fundamental insight into the production mechanism of the ROS&RNS generated by the plasma jet is achieved. With rising dissipated power the temperature and the metastable densities as well as the ozone and nitrogen dioxide concentrations are increasing. By adding molecular oxygen and nitrogen to the feed gas of a plasma jet the ROS&RNS composition can be tuned. However, also the dissipated power is changed by the small amount of admixtures. Due to the developed dissipated power measurements within this thesis it was possible to disentangle the influence of the admixture on the power and on the ROS&RNS production. If the dissipated power is fixed for the µAPPJ with argon and helium feed gas, respectively, the highest amount of ozone was measured with oxygen admixture in an argon discharge, the highest amount of dinitrogen pentoxide with nitrogen admixture in an argon discharge and the highest amount of nitrogen dioxide with nitrogen admixture in a helium discharge. Beyond the influence of the dissipated power and the molecular admixture on the ROS&RNS production the feed gas temperature is a crucial parameter for the corresponding chemical reactions. By changing this parameter the distribution of ozone and nitrogen dioxide can be tuned precisely in such a way that with increasing temperature the ozone density goes down and the nitrogen dioxide density rises. Another determinant for the ROS&RNS composition produced by an atmospheric pressure plasma jet is the influence of ambient air. If the ambient air is changing from pure nitrogen to pure oxygen atmosphere the ozone density produced by the plasma jet is increasing. For the same conditions the nitrogen dioxide has a maximum at an oxygen-to-nitrogen ratio of 1:1. To avoid the influence of the ambient air on the reactive species production the afterglow of the µAPPJ was prolonged with a glass tube. By increasing the amount of molecular admixtures to the feed gas with each in equal quantities a totally different ROS&RNS composition can be obtained compared without the glass tube. It figures out that for small molecular admixtures the reactive species composition is nitrogen dominated and for higher admixtures it is oxygen dominated. Consequently, by shielding the ambient air from the active effluent and by admixing molecular oxygen and nitrogen the ROS&RNS composition can be designed.
The content of this thesis can be summarized as follows: (i) The deposition processes of SiOx and SiOxCyHz coatings were investigated in a low-pressure, low temperature HMDSO-O2-N2 plasmas. Infrared laser absorption spectroscopy (IRLAS) and optical emission spectroscopy (OES) were combined to measure the gas temperatures in the hot and colder zones of the plasma as well as to monitor the concentration of the methyl radical, CH3, and of seven stable molecules, HMDSO, CH4, C2H2, C2H4, C2H6, CO and CO2. Tunable lead salt diode lasers (TDLs) and an external-cavity quantum cascade laser (EC-QCL) were simultaneously employed as radiation sources to perform the IRLAS measurements. They were found to be in the range between 10^{11} to 10^{15} cm^{−3}. The influence of the discharge parameters of power, pressure and gas mixture on the molecular concentrations was studied. The plasma generation is characterized by a certain degree of inhomogeneity with different temperature zones, i.e., hottest, hot and colder zones depending on the construction of the reactor. This complexity is characterized by the multiple molecular species including the HMDSO precursor and products in ground and excited states existing in the plasma. (ii) Employing similarly IRLAS and OES techniques, the deposition of nanocrystalline diamond at relatively low temperature in low-pressure MW H2 plasmas with small ad-mixtures of methane and carbon dioxide was investigated. Five methods were applied for an extensive temperature analysis, providing new insights into energetic aspects of the multi-component non-equilibrium plasma. The OES method provided information about the gas temperature of H2 inside the MW plasma. Using lead salt diode lasers, the rotational temperature of the methyl radical, CH3 , and gas temperature of methane molecule, CH4 , was measured. A variety of CO lines in the ground and in three excited states have been analysed using an EC-QCL with a relatively wide spectral range. These methods have shown that based on the construction of the DAA reactor using 16 single plasma sources the plasma generation is characterized by a variety of hottest, hot and colder zones. Extensive measurement of these various species temperatures in the complex plasma enabled the concentration determination of the various stable and unstable plasma species, which were found to be in the range between 10 11 to 10 15 cm −3 . The influence of the discharge parameters, power and pressure, on the molecular concentrations has been studied. To achieve insight into general plasma chemical aspects, the dissociation of the carbon precursor gases including their fragmentation and conversion to the reaction products was analysed in detail. The evolution of the concentration of the methyl radical, CH 3 , of five stable molecules, CH4, CO2, CO, C2H2 and C2H4, and of vibrationally excited CO in the first and second hot band was monitored in the plasma processes by in situ infrared laser absorption spectroscopy using lead salt diode lasers (TDL) and an external-cavity quantum cascade laser (EC-QCL) as radiation sources. OES was applied simultaneously to obtain complementary information about the degree of dissociation of the H2 precursor gas. The analysis of the carbon and oxygen mass balances shows clearly, that the deposition on the reactor walls and the production of other hydrocarbons species may act as sinks for carbon and oxygen. (iii) The absolute line strengths of many P-branch transitions of the ν3 fundamental of {28}^SiH4 were determined using the wide tuning range and the narrow line width of a cw EC-QCL between 2096 and 2178 cm^{−1}. The line positions and line strengths of transitions of the stretching dyad within the P-branch of {28}^SiH4 were determined with an estimated experimental measurement accuracy of 10%. The high spectral resolution available has enabled us to resolve and measure representative examples of the tetrahedral splittings associated with each component of the P-branch. The positions of these components are in excellent agreement with spherical top data system (STDS) predictions and theoretical transitions from the TDS spectroscopic database for spherical top molecules. To our knowledge, this is the first reported measurement of these line strengths in this band and is an example of the applicability of high-powered, widely tunable EC-QCLs to high resolution spectroscopy in the MIR. (iv) Similarly, the determination of the silyl radicals, ν3 band, line strengths is ongoing using the same cw EC-QCL. This effort was impaired by silane and other unknown species lines overlap; however, the silyl radicals was successfully detected in a SiH4/H2 plasma. A method to determine the silyl line strengths has been presented through its iterative decay measurements which relied on the value of the silyl radical self reaction constant. There was a consensus of its value in the literature.