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

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

scholarly journals Observations of Solar Type III Radio Bursts with the Nancay Radioheliograph

1980 ◽  
Vol 86 ◽  
pp. 235-240 ◽  
Author(s):  
M. Pick ◽  
A. Raoult ◽  
N. Vilmer
Keyword(s):  
Circular Polarization ◽  
Time Evolution ◽  
Electron Beams ◽  
Space Time ◽  
Radio Bursts ◽  
Temporal Characteristics ◽  
Type Iii ◽  
Solar Type ◽  
Space Time Evolution

Results on the space-time evolution of type III burst sources are summarized (Raoult and Pick, 1979) and observations on the temporal characteristics of the circular polarization are presented. It is shown that type III burst sources can be resolved into narrow components. Complex or very large sources may be explained by the occurrence of electron beams which propagate along different diverging paths. Propagating effects in a scattering corona are not required to explain the observations. The origin of the fundamental-harmonic pairs is briefly discussed.

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