DocumentCode :
3505026
Title :
Plasma physics challenge: confirm new plasma wave mode predicted by space physics
Author :
Benson, R.F. ; Osherovich, V.A. ; Fainberg, J. ; Reinisch, B.W.
Author_Institution :
NASA Goddard Space Flight Center, Greenbelt, MD, USA
fYear :
2004
fDate :
1-1 July 2004
Firstpage :
256
Abstract :
Summary form only given. A new plasma wave mode has been proposed to explain plasma emissions stimulated by satellite-borne high-power radio-frequency sounders designed to derive remote electron density profiles from electromagnetic-wave echoes. These sounders also generate electrostatic waves that produce coherent echoes (called plasma resonances because of their appearance on the data records) that occur near harmonics of the electron cyclotron frequency f/sub ce/, the electron plasma frequency f/sub pe/, and the upper-hybrid frequency f/sub uh/, where f/sub uh//sup 2/=f/sub pe//sup 2/+f/sub ce//sup 2/. They also stimulate plasma emissions, at frequencies related to these characteristic frequencies, including a sequence observed at frequencies below f/sub pe/ and between the f/sub ce/ harmonics. They are known as the Dn resonances because of their diffuse appearance on ionospheric topside-sounder records where they were first observed nearly forty years ago. Five mechanisms have been proposed to explain these resonances. One, based on eigenmodes of cylindrical electromagnetic plasma oscillations , predicts the observed frequency spacing of the observed Dn sequence and also that these resonances would be expected in any magnetized plasma where f/sub pe/ and f/sub ce/ are comparable. In agreement with these predictions the Dn resonances have been stimulated in other space plasmas, including the magnetosphere in spite of much different f/sub pe/, f/sub ce/ and electron temperature values, the main controlling parameter being the ratio f/sub pe//f/sub ce/. An empirical fit to ionospheric topside sounder observations yields f/sub D1/=0.95 (f/sub pe/f/sub ce/)/sup 1/2/. The main challenge remaining is to derive this fundamental frequency, i.e., for n=1 which is most prominently observed when f/sub pe//f/sub ce//spl ap/2-4, from kinetic theory (analytically or by numerical simulations) and verify using laboratory experiments.
Keywords :
astrophysical plasma; ionospheric electromagnetic wave propagation; magnetosphere; plasma density; plasma electromagnetic wave propagation; plasma hybrid waves; plasma oscillations; plasma temperature; cylindrical electromagnetic plasma oscillations; eigenmodes; electromagnetic-wave echoes; electron cyclotron frequency; electron plasma frequency; electron temperature; electrostatic wave; ionospheric topside-sounder records; magnetized plasma; magnetosphere; plasma emissions stimulation; plasma physics; plasma wave mode; remote electron density profiles; satellite-borne high-power radio-frequency sounders; space physics; space plasma; Cyclotrons; Electron emission; Electrostatics; Magnetic resonance; Magnetosphere; Physics; Plasma density; Plasma temperature; Plasma waves; Radio frequency;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Plasma Science, 2004. ICOPS 2004. IEEE Conference Record - Abstracts. The 31st IEEE International Conference on
Conference_Location :
Baltimore, MD, USA
ISSN :
0730-9244
Print_ISBN :
0-7803-8334-6
Type :
conf
DOI :
10.1109/PLASMA.2004.1339887
Filename :
1339887
Link To Document :
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