Boltzmann equation studies on electron swarm parameters in Townsend breakdown of copper vapor plasma using independently assessed electron-collision cross sections
Abstract:Electron transport coefficients in copper vapor plasma are calculated both by two-term expansion of electron Boltzmann equation Bolsig+ and tracking the random motion of electrons using Monte Carlo collision code METHES based upon recently evaluated cross section sets. The copper atoms are evaporated from hot electrode during the post-arc phase of vacuum circuit breakers, in which Townsend breakdown between electrode gaps is probable. The electron energy probability function, electron mean energy, flux/transpo… Show more
“…Since the average kinetic energy of the ectons ejected from the emitting area is a few electronvolts 38 and they are accelerated by the electric field in the sheath up to several electronvolts, inelastic collisions are dominant in the non-collapsing ion sheath, ultimately producing a Townsend breakdown. We note that Yang et al 39 investigated copper vapor plasma via simulation and reported minimum breakdown voltages of 106–122 V at . Considering that (i) the electron-impact ionization cross section of aluminum is ten times larger than those of copper and argon 40 , 41 , and (ii) the aluminum density is assumed as (few hundred millitorr of vapor pressure), breakdown is initiated within a sub-millimeter region in the non-collapsing sheath where the voltage difference between the background plasma and AIP tip is a few hundred volts.…”
Arcing is a ubiquitous phenomenon and a crucial issue in high-voltage applied systems, especially low-temperature plasma (LTP) engineering. Although arcing in LTPs has attracted interest due to the severe damage it can cause, its underlying mechanism has yet to be fully understood. To elucidate the arcing mechanism, this study investigated various signals conventionally used to analyze arcing such as light emission, arcing current and voltage, and background plasma potential. As a result, we found that light emission occurs as early as 0.56 μs before arcing current initiation, which is a significant indicator of the explosive development of arcing as well as other signals. We introduce an arcing inducing probe (AIP) designed to localize arcing on the tip edge along with multiple snapshot analysis since arcing occurs randomly in space and time. Analysis reveals that the prior light emission consists of sheath and tip glows from the whole AIP sheath and the AIP tip edge, respectively. Formation mechanisms of these emissions based on multiple snapshot image analysis are discussed. This light emission before arcing current initiation provides a significant clue to understanding the arcing formation mechanism and represents a new indicator for forecasting arcing in LTPs.
“…Since the average kinetic energy of the ectons ejected from the emitting area is a few electronvolts 38 and they are accelerated by the electric field in the sheath up to several electronvolts, inelastic collisions are dominant in the non-collapsing ion sheath, ultimately producing a Townsend breakdown. We note that Yang et al 39 investigated copper vapor plasma via simulation and reported minimum breakdown voltages of 106–122 V at . Considering that (i) the electron-impact ionization cross section of aluminum is ten times larger than those of copper and argon 40 , 41 , and (ii) the aluminum density is assumed as (few hundred millitorr of vapor pressure), breakdown is initiated within a sub-millimeter region in the non-collapsing sheath where the voltage difference between the background plasma and AIP tip is a few hundred volts.…”
Arcing is a ubiquitous phenomenon and a crucial issue in high-voltage applied systems, especially low-temperature plasma (LTP) engineering. Although arcing in LTPs has attracted interest due to the severe damage it can cause, its underlying mechanism has yet to be fully understood. To elucidate the arcing mechanism, this study investigated various signals conventionally used to analyze arcing such as light emission, arcing current and voltage, and background plasma potential. As a result, we found that light emission occurs as early as 0.56 μs before arcing current initiation, which is a significant indicator of the explosive development of arcing as well as other signals. We introduce an arcing inducing probe (AIP) designed to localize arcing on the tip edge along with multiple snapshot analysis since arcing occurs randomly in space and time. Analysis reveals that the prior light emission consists of sheath and tip glows from the whole AIP sheath and the AIP tip edge, respectively. Formation mechanisms of these emissions based on multiple snapshot image analysis are discussed. This light emission before arcing current initiation provides a significant clue to understanding the arcing formation mechanism and represents a new indicator for forecasting arcing in LTPs.
“…. Researches [51,52] suggest, that background VDF becomes important in the case of small fields. The latter can be taken into account by changing u 0 term in (8): u 0 → u 0 + v bg , where v bg corresponds to thermal velocity, sampled from the background VDF.…”
In this paper, we examine the energy distribution function of electrons in the case of a very weakly ionized
argon plasma at sub-atmospheric pressure and external electric field using Boltzmann kinetic equation. We are
interested in the behavior of the collisional part of the equation, thus spatially uniform model is considered. The
goal of the research is to compare two different numerical approaches: a deterministic one (using a two-term local
non-stationary approximation) and a stochastic approach (using the Monte Carlo method) over a wide range of
reduced electric fields: from several Td to kTd. We present the comparison for steady-state and time-dependent
solutions, isotropic and anisotropic parts of the electron energy distribution function, and reaction constants.
The research will also help to identify any limitations and challenges of these methods.
“…The left panel shows the elastic momentum transfer (1), total ionization (2), and quantities that are obtained by multiplying the total cross section for superelastic collisions with the corresponding fractional populations of the first excited metastable state at indium vapour temperatures of 1260 K, 3260 K, and 5260 K. The left panel also includes the following discrete inelastic transitions: (5s 2 5p) 2 P 3/2 (3), (5s 2 6s) 2 S 1/2 (4), (5s 2 6p) 2 P 1/2 (5), (5s 2 6p) 2 P 3/2 (6), (5s 2 5d) 2 D 3/2 (7), (5s 2 5d) 2 D 5/2 (8), (5s 2 4p) 2 P 1/2 (9), (5s 2 4p) 2 P 3/2 (10), (5s 2 7s) 2 S 1/2 (11) and (5s 2 4p) 2 P 5/2 (12). The right panel includes the following discrete inelastic transitions: (5s 2 7s) 2 P 1/2 (13), (5s 2 7s) 2 P 3/2 (14), (5p 2 6d) 2 D 3/2 (15), (5p 2 6d) 2 D 5/2 (16), (5p 2 4 f ) 2 F 7/2 (17), (5p 2 4 f ) 2 F 5/2 (18), (5p 2 8s) 2 S 1/2 (19), (5p 2 8s) 2 P 1/2 (20), (5s 2 7d) 2 D 3/2 (21), (5s 2 7d) 2 D 5/2 (22) and (5s 2 8p) 2 P 3/2 (23). Integral cross sections for electron scattering in indium vapour for atoms in the metastable state (5s 2 5p) 2 P 3/2 .…”
Section: Monte Carlo Simulationsmentioning
confidence: 99%
“…The primary driving force behind these early studies was the modelling and optimization of light sources containing mercury [8,14,15], sodium [16,17], and zinc [18,19]. Other applications include the modelling of a gas laser [20], the magnetohydrodynamics of arcs [21], and a post-arc breakdown plasma [22].…”
Section: Introductionmentioning
confidence: 99%
“…The computed cross-sections were subsequently used as input to solve the Boltzmann equation to calculate the electron swarm transport coefficients. The publicly available two-term Boltzmann equation solver BOLSIG+ [27], as well as the Monte Carlo code METHES [28], were recently used to investigate the electron transport and breakdown in a copper vapour post-arc plasma [22]. The relativistic complex optical potential method has also been used to study electron-beryllium scattering [29].…”
We study the transport of electrons and propagation of the negative ionisation fronts in indium vapour. Electron swarm transport properties are calculated using a Monte Carlo simulation technique over a wide range of reduced electric fields E/N (where E is the electric field and N is the gas number density) and indium vapour temperatures in hydrodynamic conditions, and under non-hydrodynamic conditions in an idealised steady-state Townsend (SST) setup. As many indium atoms are in the first
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metastable state at vapour temperatures of a few thousand Kelvin, the initial Monte Carlo code was extended and generalized to consider the spatial relaxation and the transport of electrons in an idealised SST experiment, in the presence of thermal motion of the host-gas atoms and superelastic collisions. We observe a significant sensitivity of the spatial relaxation of the electrons on the indium vapour temperature and the initial conditions used to release electrons from the cathode into the space between the electrodes. The calculated electron transport coefficients are used as input for the classical fluid model, to investigate the inception and propagation of negative ionisation fronts in indium vapour at various E/N and vapour temperatures. We calculate the electron density, electric field, and velocity of ionisation fronts as a function of E/N and indium vapour temperature. The presence of indium atoms in the first
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metastable state significantly affects the characteristics of the negative ionisation fronts. The transition from an avalanche into a negative ionisation front occurs faster with increasing indium vapour temperature, due to enhanced ionisation and more efficient production of electrons at higher vapour temperatures. For lower values of E/N, the electron density behind the streamer front, where the electric field is screened, does not decay as one might expect for atomic gases, but it could be increased due to the accumulation of low-energy electrons that are capable of initiating ionisation in the streamer interior.
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