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Electron acceleration during streamer collisions in air

High‐voltage laboratory experiments show that discharges in air, generated over a gap of one meter with maximal voltage of 1 MV, may produce X‐rays with photon energies up to 1 MeV. It has been suggested that the photons are bremsstrahlung from electrons accelerated by the impulsive, enhanced field...

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Autores principales: Köhn, Christoph, Chanrion, Olivier, Neubert, Torsten
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2017
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5405581/
https://www.ncbi.nlm.nih.gov/pubmed/28503005
http://dx.doi.org/10.1002/2016GL072216
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author Köhn, Christoph
Chanrion, Olivier
Neubert, Torsten
author_facet Köhn, Christoph
Chanrion, Olivier
Neubert, Torsten
author_sort Köhn, Christoph
collection PubMed
description High‐voltage laboratory experiments show that discharges in air, generated over a gap of one meter with maximal voltage of 1 MV, may produce X‐rays with photon energies up to 1 MeV. It has been suggested that the photons are bremsstrahlung from electrons accelerated by the impulsive, enhanced field during collisions of negative and a positive streamers. To explore this process, we have conducted the first self‐consistent particle simulations of streamer encounters. Our simulation model is a 2‐D, cylindrically symmetric, particle‐in‐cell code tracing the electron dynamics and solving the space charge fields, with a Monte Carlo scheme accounting for collisions and ionization. We present the electron density, the electric field, and the velocity distribution as functions of space and time. Assuming a background electric field 1.5 times the breakdown field, we find that the electron density reaches 2·10(21) m(−3), the size of the encounter region is ∼3·10(−12) m(3) and that the field enhances to ∼9 times the breakdown field during ∼10(−11) s. We further find that the radial component becomes comparable to the parallel component, which together with angular scattering leads to an almost isotropic distribution of electrons. This is consistent with laboratory observations that X‐rays are emitted isotropically. However, the maximum energy of electrons reached in the simulation is ∼600 eV, which is well below the energies required to explain observations. The reason is that the encounter region is small in size and duration. For the photon energies observed, the field must be enhanced in a larger region and/or for a longer time.
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spelling pubmed-54055812017-05-11 Electron acceleration during streamer collisions in air Köhn, Christoph Chanrion, Olivier Neubert, Torsten Geophys Res Lett Research Letters High‐voltage laboratory experiments show that discharges in air, generated over a gap of one meter with maximal voltage of 1 MV, may produce X‐rays with photon energies up to 1 MeV. It has been suggested that the photons are bremsstrahlung from electrons accelerated by the impulsive, enhanced field during collisions of negative and a positive streamers. To explore this process, we have conducted the first self‐consistent particle simulations of streamer encounters. Our simulation model is a 2‐D, cylindrically symmetric, particle‐in‐cell code tracing the electron dynamics and solving the space charge fields, with a Monte Carlo scheme accounting for collisions and ionization. We present the electron density, the electric field, and the velocity distribution as functions of space and time. Assuming a background electric field 1.5 times the breakdown field, we find that the electron density reaches 2·10(21) m(−3), the size of the encounter region is ∼3·10(−12) m(3) and that the field enhances to ∼9 times the breakdown field during ∼10(−11) s. We further find that the radial component becomes comparable to the parallel component, which together with angular scattering leads to an almost isotropic distribution of electrons. This is consistent with laboratory observations that X‐rays are emitted isotropically. However, the maximum energy of electrons reached in the simulation is ∼600 eV, which is well below the energies required to explain observations. The reason is that the encounter region is small in size and duration. For the photon energies observed, the field must be enhanced in a larger region and/or for a longer time. John Wiley and Sons Inc. 2017-03-15 2017-03-16 /pmc/articles/PMC5405581/ /pubmed/28503005 http://dx.doi.org/10.1002/2016GL072216 Text en ©2017. The Authors. This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs (http://creativecommons.org/licenses/by-nc-nd/4.0/) License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.
spellingShingle Research Letters
Köhn, Christoph
Chanrion, Olivier
Neubert, Torsten
Electron acceleration during streamer collisions in air
title Electron acceleration during streamer collisions in air
title_full Electron acceleration during streamer collisions in air
title_fullStr Electron acceleration during streamer collisions in air
title_full_unstemmed Electron acceleration during streamer collisions in air
title_short Electron acceleration during streamer collisions in air
title_sort electron acceleration during streamer collisions in air
topic Research Letters
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5405581/
https://www.ncbi.nlm.nih.gov/pubmed/28503005
http://dx.doi.org/10.1002/2016GL072216
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