Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheet

In this study we perform a statistical survey of the extremely-low-frequency wave activities associated with fast earthward flows in the mid-tail central plasma sheet (CPS) based upon THEMIS measurements. We reveal clear trends of increasing wave intensity with flow enhancement over a broad freq...

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Main Authors: J. Liang, B. Ni, C. M. Cully, E. F. Donovan, R. M. Thorne, V. Angelopoulos
Format: Article
Language:English
Published: Copernicus Publications 2012-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/30/467/2012/angeo-30-467-2012.pdf
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spelling doaj-b670234eca4b46bb8d454332759d6c8b2020-11-24T21:02:56ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762012-03-013046748810.5194/angeo-30-467-2012Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheetJ. Liang0B. Ni1C. M. Cully2E. F. Donovan3R. M. Thorne4V. Angelopoulos5V. Angelopoulos6Dept. of Physics and Astronomy, Univ. of Calgary, CanadaDept. of Atmospheric and Oceanic Sciences, UCLA, CA, USASwedish Institute of Space Physics, Uppsala, SwedenDept. of Physics and Astronomy, Univ. of Calgary, CanadaDept. of Atmospheric and Oceanic Sciences, UCLA, CA, USAInstitute of Geophysics and Planetary Physics, UCLA, CA, USAEarth and Space Sciences Department, UCLA, CA, USAIn this study we perform a statistical survey of the extremely-low-frequency wave activities associated with fast earthward flows in the mid-tail central plasma sheet (CPS) based upon THEMIS measurements. We reveal clear trends of increasing wave intensity with flow enhancement over a broad frequency range, from below <I>f</I><sub>LH</sub> (lower-hybrid resonant frequency) to above <I>f</I><sub>ce</sub> (electron gyrofrequency). We mainly investigate two electromagnetic wave modes, the lower-hybrid waves at frequencies below <I>f</I><sub>LH</sub>, and the whistler-mode waves in the frequency range <I>f</I><sub>LH</sub> < <I>f</I> < <I>f</I><sub>ce</sub>. The waves at <I>f</I> < <I>f</I><sub>LH</sub> dramatically intensify during fast flow intervals, and tend to contain strong electromagnetic components in the high-plasma-beta CPS region, consistent with the theoretical expectation of the lower-hybrid drift instability in the center region of the tail current sheet. ULF waves with very large perpendicular wavenumber might be Doppler-shifted by the flows and also partly contribute to the observed waves in the lower-hybrid frequency range. The fast flow activity substantially increases the occurrence rate and peak magnitude of the electromagnetic waves in the frequency range <I>f</I><sub>LH</sub> < <I>f</I> < <I>f</I><sub>ce</sub>, though they still tend to be short-lived and sporadic in occurrence. We also find that the electron pitch-angle distribution in the mid-tail CPS undergoes a variation from negative anisotropy (perpendicular temperature smaller than parallel temperature) during weak flow intervals, to more or less positive anisotropy (perpendicular temperature larger than parallel temperature) during fast flow intervals. The flow-related electromagnetic whistler-mode wave tends to occur in conjunction with positive electron anisotropy.https://www.ann-geophys.net/30/467/2012/angeo-30-467-2012.pdf
collection DOAJ
language English
format Article
sources DOAJ
author J. Liang
B. Ni
C. M. Cully
E. F. Donovan
R. M. Thorne
V. Angelopoulos
V. Angelopoulos
spellingShingle J. Liang
B. Ni
C. M. Cully
E. F. Donovan
R. M. Thorne
V. Angelopoulos
V. Angelopoulos
Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheet
Annales Geophysicae
author_facet J. Liang
B. Ni
C. M. Cully
E. F. Donovan
R. M. Thorne
V. Angelopoulos
V. Angelopoulos
author_sort J. Liang
title Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheet
title_short Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheet
title_full Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheet
title_fullStr Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheet
title_full_unstemmed Electromagnetic ELF wave intensification associated with fast earthward flows in mid-tail plasma sheet
title_sort electromagnetic elf wave intensification associated with fast earthward flows in mid-tail plasma sheet
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2012-03-01
description In this study we perform a statistical survey of the extremely-low-frequency wave activities associated with fast earthward flows in the mid-tail central plasma sheet (CPS) based upon THEMIS measurements. We reveal clear trends of increasing wave intensity with flow enhancement over a broad frequency range, from below <I>f</I><sub>LH</sub> (lower-hybrid resonant frequency) to above <I>f</I><sub>ce</sub> (electron gyrofrequency). We mainly investigate two electromagnetic wave modes, the lower-hybrid waves at frequencies below <I>f</I><sub>LH</sub>, and the whistler-mode waves in the frequency range <I>f</I><sub>LH</sub> < <I>f</I> < <I>f</I><sub>ce</sub>. The waves at <I>f</I> < <I>f</I><sub>LH</sub> dramatically intensify during fast flow intervals, and tend to contain strong electromagnetic components in the high-plasma-beta CPS region, consistent with the theoretical expectation of the lower-hybrid drift instability in the center region of the tail current sheet. ULF waves with very large perpendicular wavenumber might be Doppler-shifted by the flows and also partly contribute to the observed waves in the lower-hybrid frequency range. The fast flow activity substantially increases the occurrence rate and peak magnitude of the electromagnetic waves in the frequency range <I>f</I><sub>LH</sub> < <I>f</I> < <I>f</I><sub>ce</sub>, though they still tend to be short-lived and sporadic in occurrence. We also find that the electron pitch-angle distribution in the mid-tail CPS undergoes a variation from negative anisotropy (perpendicular temperature smaller than parallel temperature) during weak flow intervals, to more or less positive anisotropy (perpendicular temperature larger than parallel temperature) during fast flow intervals. The flow-related electromagnetic whistler-mode wave tends to occur in conjunction with positive electron anisotropy.
url https://www.ann-geophys.net/30/467/2012/angeo-30-467-2012.pdf
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