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

Source at https://doi.org/10.1007/s00585-998-1226-z 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 sepa...

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Published in:Annales Geophysicae
Main Authors: Guio, Patrick, Lilensten, J., Kofman, W., Bjørnå, Noralv
Format: Article in Journal/Newspaper
Language:English
Published: European Geophysical Society 1998
Subjects:
Online Access:https://hdl.handle.net/10037/555
https://doi.org/10.1007/s00585-998-1226-z
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author Guio, Patrick
Lilensten, J.
Kofman, W.
Bjørnå, Noralv
author_facet Guio, Patrick
Lilensten, J.
Kofman, W.
Bjørnå, Noralv
author_sort Guio, Patrick
collection University of Tromsø: Munin Open Research Archive
container_issue 10
container_start_page 1226
container_title Annales Geophysicae
container_volume 16
description Source at https://doi.org/10.1007/s00585-998-1226-z 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.
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genre_facet EISCAT
geographic Langmuir
geographic_facet Langmuir
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op_doi https://doi.org/10.1007/s00585-998-1226-z
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spelling ftunivtroemsoe:oai:munin.uit.no:10037/555 2025-04-13T14:18:07+00:00 Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines. Guio, Patrick Lilensten, J. Kofman, W. Bjørnå, Noralv 1998-10-31 2875697 bytes application/pdf https://hdl.handle.net/10037/555 https://doi.org/10.1007/s00585-998-1226-z eng eng European Geophysical Society https://hdl.handle.net/10037/555 openAccess Non-Maxwellian electron velocity distribution Incoherent scatter plasma lines Eiscat Dielectric response function VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme akustikk optikk: 434 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437 Journal article Tidsskriftartikkel 1998 ftunivtroemsoe https://doi.org/10.1007/s00585-998-1226-z 2025-03-14T05:17:55Z Source at https://doi.org/10.1007/s00585-998-1226-z 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. Article in Journal/Newspaper EISCAT University of Tromsø: Munin Open Research Archive Langmuir ENVELOPE(-67.150,-67.150,-66.967,-66.967) Annales Geophysicae 16 10 1226 1240
spellingShingle Non-Maxwellian electron velocity distribution
Incoherent scatter plasma lines
Eiscat
Dielectric response function
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
Guio, Patrick
Lilensten, J.
Kofman, W.
Bjørnå, Noralv
Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines.
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_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_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_sort electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines.
topic Non-Maxwellian electron velocity distribution
Incoherent scatter plasma lines
Eiscat
Dielectric response function
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
topic_facet Non-Maxwellian electron velocity distribution
Incoherent scatter plasma lines
Eiscat
Dielectric response function
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Elektromagnetisme
akustikk
optikk: 434
VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
url https://hdl.handle.net/10037/555
https://doi.org/10.1007/s00585-998-1226-z