Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines

The plasma dispersion function and the reduced velocity distribution function are calculated numerically for any arbitrary velocity distribution function with cylindrical symmetry along the magnetic field. The electron velocity distribution is separated into two distributions representing the distri...

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Published in:Annales Geophysicae
Main Authors: Guio, P., Lilensten, J., Kofman, W., Bjørnå, N.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.1007/s00585-998-1226-z
https://angeo.copernicus.org/articles/16/1226/1998/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo34220 2023-05-15T16:04:48+02:00 Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines Guio, P. Lilensten, J. Kofman, W. Bjørnå, N. 2018-09-27 application/pdf https://doi.org/10.1007/s00585-998-1226-z https://angeo.copernicus.org/articles/16/1226/1998/ eng eng doi:10.1007/s00585-998-1226-z https://angeo.copernicus.org/articles/16/1226/1998/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.1007/s00585-998-1226-z 2020-07-20T16:28:05Z The plasma dispersion function and the reduced velocity distribution function are calculated numerically for any arbitrary velocity distribution function with cylindrical symmetry along the magnetic field. The electron velocity distribution is separated into two distributions representing the distribution of the ambient electrons and the suprathermal electrons. The velocity distribution function of the ambient electrons is modelled by a near-Maxwellian distribution function in presence of a temperature gradient and a potential electric field. The velocity distribution function of the suprathermal electrons is derived from a numerical model of the angular energy flux spectrum obtained by solving the transport equation of electrons. The numerical method used to calculate the plasma dispersion function and the reduced velocity distribution is described. The numerical code is used with simulated data to evaluate the Doppler frequency asymmetry between the up- and downshifted plasma lines of the incoherent-scatter plasma lines at different wave vectors. It is shown that the observed Doppler asymmetry is more dependent on deviation from the Maxwellian through the thermal part for high-frequency radars, while for low-frequency radars the Doppler asymmetry depends more on the presence of a suprathermal population. It is also seen that the full evaluation of the plasma dispersion function gives larger Doppler asymmetry than the heat flow approximation for Langmuir waves with phase velocity about three to six times the mean thermal velocity. For such waves the moment expansion of the dispersion function is not fully valid and the full calculation of the dispersion function is needed. Key words. Non-Maxwellian electron velocity distribution · Incoherent scatter plasma lines · EISCAT · Dielectric response function Text EISCAT Copernicus Publications: E-Journals Langmuir ENVELOPE(-67.150,-67.150,-66.967,-66.967) Annales Geophysicae 16 10 1226 1240
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The plasma dispersion function and the reduced velocity distribution function are calculated numerically for any arbitrary velocity distribution function with cylindrical symmetry along the magnetic field. The electron velocity distribution is separated into two distributions representing the distribution of the ambient electrons and the suprathermal electrons. The velocity distribution function of the ambient electrons is modelled by a near-Maxwellian distribution function in presence of a temperature gradient and a potential electric field. The velocity distribution function of the suprathermal electrons is derived from a numerical model of the angular energy flux spectrum obtained by solving the transport equation of electrons. The numerical method used to calculate the plasma dispersion function and the reduced velocity distribution is described. The numerical code is used with simulated data to evaluate the Doppler frequency asymmetry between the up- and downshifted plasma lines of the incoherent-scatter plasma lines at different wave vectors. It is shown that the observed Doppler asymmetry is more dependent on deviation from the Maxwellian through the thermal part for high-frequency radars, while for low-frequency radars the Doppler asymmetry depends more on the presence of a suprathermal population. It is also seen that the full evaluation of the plasma dispersion function gives larger Doppler asymmetry than the heat flow approximation for Langmuir waves with phase velocity about three to six times the mean thermal velocity. For such waves the moment expansion of the dispersion function is not fully valid and the full calculation of the dispersion function is needed. Key words. Non-Maxwellian electron velocity distribution · Incoherent scatter plasma lines · EISCAT · Dielectric response function
format Text
author Guio, P.
Lilensten, J.
Kofman, W.
Bjørnå, N.
spellingShingle Guio, P.
Lilensten, J.
Kofman, W.
Bjørnå, N.
Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
author_facet Guio, P.
Lilensten, J.
Kofman, W.
Bjørnå, N.
author_sort Guio, P.
title Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
title_short Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
title_full Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
title_fullStr Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
title_full_unstemmed Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
title_sort electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
publishDate 2018
url https://doi.org/10.1007/s00585-998-1226-z
https://angeo.copernicus.org/articles/16/1226/1998/
long_lat ENVELOPE(-67.150,-67.150,-66.967,-66.967)
geographic Langmuir
geographic_facet Langmuir
genre EISCAT
genre_facet EISCAT
op_source eISSN: 1432-0576
op_relation doi:10.1007/s00585-998-1226-z
https://angeo.copernicus.org/articles/16/1226/1998/
op_doi https://doi.org/10.1007/s00585-998-1226-z
container_title Annales Geophysicae
container_volume 16
container_issue 10
container_start_page 1226
op_container_end_page 1240
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