Electron plasma oscillations associated with type III radio emissions and solar electrons

Solar Physics ◽  
1975 ◽  
Vol 45 (2) ◽  
pp. 477-493 ◽  
Author(s):  
D. A. Gurnett ◽  
L. A. Frank
1980 ◽  
Vol 86 ◽  
pp. 327-327 ◽  
Author(s):  
G.V. de Genouillac ◽  
D.F. Escande

Type III solar radio bursts are known to be excited by solar electron clouds travelling outwards through the solar corona and interplanetary medium. According to the “plasma hypothesis”, electron plasma oscillations are created by the passing beam, which are in turn converted into electromagnetic waves.


Science ◽  
1976 ◽  
Vol 194 (4270) ◽  
pp. 1159-1162 ◽  
Author(s):  
D. A. GURNETT ◽  
R. R. ANDERSON

2009 ◽  
Vol 76 (1) ◽  
pp. 7-17 ◽  
Author(s):  
BENGT ELIASSON ◽  
PADMA KANT SHUKLA

AbstractWe present a derivation of the dispersion relation for electrostatic oscillations in a zero-temperature quantum plasma, in which degenerate electrons are governed by the Wigner equation, while non-degenerate ions follow the classical fluid equations. The Poisson equation determines the electrostatic wave potential. We consider parameters ranging from semiconductor plasmas to metallic plasmas and electron densities of compressed matter such as in laser compression schemes and dense astrophysical objects. Owing to the wave diffraction caused by overlapping electron wave function because of the Heisenberg uncertainty principle in dense plasmas, we have the possibility of Landau damping of the high-frequency electron plasma oscillations at large enough wavenumbers. The exact dispersion relations for the electron plasma oscillations are solved numerically and compared with the ones obtained by using approximate formulas for the electron susceptibility in the high- and low-frequency cases.


1990 ◽  
Vol 17 (11) ◽  
pp. 1805-1808 ◽  
Author(s):  
G. K. Crawford ◽  
R. J. Strangeway ◽  
C. T. Russell

2019 ◽  
Vol 26 (2) ◽  
pp. 022112 ◽  
Author(s):  
Hui Xu ◽  
Fu-fang Su ◽  
Xiang-mu Kong ◽  
Yu Sun ◽  
Rui-ning Jin ◽  
...  

1999 ◽  
Vol 26 (3) ◽  
pp. 397-400 ◽  
Author(s):  
M. J. Reiner ◽  
M. L. Kaiser

2008 ◽  
Vol 113 (A7) ◽  
pp. n/a-n/a ◽  
Author(s):  
F. Duru ◽  
D. A. Gurnett ◽  
D. D. Morgan ◽  
R. Modolo ◽  
A. F. Nagy ◽  
...  

1980 ◽  
Vol 86 ◽  
pp. 299-302
Author(s):  
T. Takakura

By the use of semi-analytical method, modeling of three kinds of type III solar radio bursts have been made. Many basic problems about the type III bursts and associated solar electrons have been solved showing some striking or unexpected results. If the fundamental radio emissions should be really observed as the normal type III bursts, the emission mechanism would not be the currently accepted one, i.e. the scattering of plasma waves by ions.


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