scholarly journals Simulation on Generation of Electromagnetic Waves from Electron Beam: Application to Solar Type III Radio Bursts

2000 ◽  
Vol 138 ◽  
pp. 724-725 ◽  
Author(s):  
Daisuke Sugiyama ◽  
Jun-Ichi Sakai ◽  
Mitsuhiro Nambu
Keyword(s):  
Electron Beam ◽  
Electromagnetic Waves ◽  
Radio Bursts ◽  
Type Iii ◽  
Solar Type

scholarly journals The effect of electron beam pitch angle and density gradient on solar type III radio bursts

2012 ◽  
Vol 19 (11) ◽  
pp. 112903 ◽  
Author(s):  
R. Pechhacker ◽  
D. Tsiklauri
Keyword(s):  
Electron Beam ◽  
Density Gradient ◽  
Pitch Angle ◽  
Radio Bursts ◽  
Type Iii ◽  
Solar Type

Wave-wave interactions in solar type III radio bursts

2014 ◽  
Author(s):  
G. Thejappa ◽  
R. J. MacDowall
Keyword(s):  
Radio Bursts ◽  
Wave Interactions ◽  
Type Iii ◽  
Solar Type

WindSpacecraft Observations of Solar Impulsive Electron Events Associated with Solar Type III Radio Bursts

1998 ◽  
Vol 503 (1) ◽  
pp. 435-445 ◽  
Author(s):  
R. E. Ergun ◽  
D. Larson ◽  
R. P. Lin ◽  
J. P. McFadden ◽  
C. W. Carlson ◽  
...  
Keyword(s):  
Radio Bursts ◽  
Type Iii ◽  
Solar Type

EVIDENCE AGAINST THE OSCILLATING TWO-STREAM INSTABILITY AND SPATIAL COLLAPSE OF LANGMUIR WAVES IN SOLAR TYPE III RADIO BURSTS

2012 ◽  
Vol 753 (1) ◽  
pp. L18 ◽  
Author(s):  
D. B. Graham ◽  
Iver H. Cairns ◽  
D. M. Malaspina ◽  
R. E. Ergun
Keyword(s):  
Radio Bursts ◽  
Langmuir Waves ◽  
Type Iii ◽  
Solar Type ◽  
Stream Instability

scholarly journals Distribution Functions of Type III Electrons Observed in Interplanetary Space

1980 ◽  
Vol 86 ◽  
pp. 311-313
Author(s):  
R. P. Lin ◽  
D. W. Potter ◽  
K. A. Anderson ◽  
J. Fainberg ◽  
R. G. Stone ◽  
...  
Keyword(s):  
Pitch Angle ◽  
Energetic Particle ◽  
Solar Radio ◽  
Interplanetary Space ◽  
Energetic Electron ◽  
Distribution Functions ◽  
Radio Bursts ◽  
Type Iii ◽  
Solar Type ◽  
Good Energy

We present simultaneous energetic electron and solar radio observations from the ISEE−3 spacecraft of several solar type III radio bursts. The UC Berkeley energetic particle experiment measures from 2 to ~ 103 keV with good energy and pitch angle resolution while the Meudon/GSFC radio experiment tracks type III radio bursts at 24 frequencies in the range 30 kHz—2 MHz.

Nonlinear stability of solar type III radio bursts. I - Theory

1979 ◽  
Vol 234 ◽  
pp. 348 ◽  
Author(s):  
R. A. Smith ◽  
M. L. Goldstein ◽  
K. Papadopoulos
Keyword(s):  
Nonlinear Stability ◽  
Radio Bursts ◽  
Type Iii ◽  
Solar Type

Proceedings of the workshop on mechanisms for solar type III radio bursts

Solar Physics ◽  
1976 ◽  
Vol 46 (2) ◽  
pp. 433-435 ◽  
Author(s):  
R. P. Lin
Keyword(s):  
Radio Bursts ◽  
Type Iii ◽  
Solar Type
Sign in / Sign up

Export Citation Format

Share Document