Wave-wave interactions in solar type III radio bursts

Author(s):  
G. Thejappa ◽  
R. J. MacDowall
1986 ◽  
Vol 308 ◽  
pp. 954 ◽  
Author(s):  
R. P. Lin ◽  
W. K. Levedahl ◽  
W. Lotko ◽  
D. A. Gurnett ◽  
F. L. Scarf

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):  
Type Iii ◽  

1980 ◽  
Vol 86 ◽  
pp. 311-313
Author(s):  
R. P. Lin ◽  
D. W. Potter ◽  
K. A. Anderson ◽  
J. Fainberg ◽  
R. G. Stone ◽  
...  

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.


1979 ◽  
Vol 234 ◽  
pp. 348 ◽  
Author(s):  
R. A. Smith ◽  
M. L. Goldstein ◽  
K. Papadopoulos

2000 ◽  
Vol 179 ◽  
pp. 447-450
Author(s):  
G. Thejappa ◽  
R. J. MacDowall

AbstractThe Ulysses Unified Radio and Plasma Wave Experiment (URAP) has observed Langmuir, ion-acoustic and associated solar type III radio emissions in the interplanetary medium. Bursts of 50–300 Hz (in the spacecraft frame) electric field signals, corresponding to long-wavelength ion-acoustic waves are often observed coincident in time with the most intense Langmuir wave spikes, providing evidence for the electrostatic decay instability. Langmuir waves often occur as envelope solitons, suggesting that strong turbulence processes, such as modulational instability and soliton formation, often coexist with weak turbulence processes, such as electrostatic decay, in a few type III burst source regions.


Sign in / Sign up

Export Citation Format

Share Document