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...

Full description

Bibliographic Details
Published in:Annales Geophysicae
Main Authors: P. Guio, J. Lilensten, W. Kofman, N. Bjørnå
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 1998
Subjects:
Q
Online Access:https://doi.org/10.1007/s00585-998-1226-z
https://doaj.org/article/0608853ed7cf40b382c6566193cb5aae
id ftdoajarticles:oai:doaj.org/article:0608853ed7cf40b382c6566193cb5aae
record_format openpolar
spelling ftdoajarticles:oai:doaj.org/article:0608853ed7cf40b382c6566193cb5aae 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 P. Guio J. Lilensten W. Kofman N. Bjørnå 1998-10-01T00:00:00Z https://doi.org/10.1007/s00585-998-1226-z https://doaj.org/article/0608853ed7cf40b382c6566193cb5aae EN eng Copernicus Publications https://www.ann-geophys.net/16/1226/1998/angeo-16-1226-1998.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.1007/s00585-998-1226-z 0992-7689 1432-0576 https://doaj.org/article/0608853ed7cf40b382c6566193cb5aae Annales Geophysicae, Vol 16, Pp 1226-1240 (1998) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 1998 ftdoajarticles https://doi.org/10.1007/s00585-998-1226-z 2022-12-30T22:15:44Z 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 Article in Journal/Newspaper EISCAT Directory of Open Access Journals: DOAJ Articles Langmuir ENVELOPE(-67.150,-67.150,-66.967,-66.967) Annales Geophysicae 16 10 1226 1240
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
spellingShingle Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
P. Guio
J. Lilensten
W. Kofman
N. Bjørnå
Electron velocity distribution function in a plasma with temperature gradient and in the presence of suprathermal electrons: application to incoherent-scatter plasma lines
topic_facet Science
Q
Physics
QC1-999
Geophysics. Cosmic physics
QC801-809
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 Article in Journal/Newspaper
author P. Guio
J. Lilensten
W. Kofman
N. Bjørnå
author_facet P. Guio
J. Lilensten
W. Kofman
N. Bjørnå
author_sort P. Guio
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
publisher Copernicus Publications
publishDate 1998
url https://doi.org/10.1007/s00585-998-1226-z
https://doaj.org/article/0608853ed7cf40b382c6566193cb5aae
long_lat ENVELOPE(-67.150,-67.150,-66.967,-66.967)
geographic Langmuir
geographic_facet Langmuir
genre EISCAT
genre_facet EISCAT
op_source Annales Geophysicae, Vol 16, Pp 1226-1240 (1998)
op_relation https://www.ann-geophys.net/16/1226/1998/angeo-16-1226-1998.pdf
https://doaj.org/toc/0992-7689
https://doaj.org/toc/1432-0576
doi:10.1007/s00585-998-1226-z
0992-7689
1432-0576
https://doaj.org/article/0608853ed7cf40b382c6566193cb5aae
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
_version_ 1766400437698691072