scholarly journals A superfine structure in solar microwave bursts

2003 ◽  
Vol 406 (3) ◽  
pp. 1071-1081 ◽  
Author(s):  
G. P. Chernov ◽  
Y. H. Yan ◽  
Q. J. Fu

2007 ◽  
Vol 33 (5) ◽  
pp. 319-326 ◽  
Author(s):  
A. A. Kuznetsov






1960 ◽  
Vol 65 ◽  
pp. 50
Author(s):  
M. H. Cohen


Solar Physics ◽  
1986 ◽  
Vol 104 (2) ◽  
pp. 391-413 ◽  
Author(s):  
S. Z. Jin ◽  
R. Y. Zhao ◽  
Q. J. Fu


1997 ◽  
Vol 481 (1) ◽  
pp. 532-544 ◽  
Author(s):  
L. Belkora


1972 ◽  
Vol 178 ◽  
pp. 241 ◽  
Author(s):  
Reuven Ramaty ◽  
Vahe Petrosian


1985 ◽  
Vol 292 ◽  
pp. 733 ◽  
Author(s):  
R. K. Shevgaonkar ◽  
M. R. Kundu


1993 ◽  
Vol 141 ◽  
pp. 295-298
Author(s):  
Ren-Yang Zhao

AbstractBased on the theory of gyro-synchrotron radiation from both thermal and nonthermal electrons, and adopting the relation between the peak frequency and the corresponding rise time of microwave bursts, we have derived several analytical formulae for calculating the magnetic field in the source regions of solar microwave bursts.



Nature ◽  
1970 ◽  
Vol 226 (5240) ◽  
pp. 68-69 ◽  
Author(s):  
REUVEN RAMATY ◽  
STEPHEN S. HOLT


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