Microwave Sources of Solar Flares: Loop Top or Foot Points?

Author(s):  
Keizo Kai
1980 ◽  
Vol 86 ◽  
pp. 443-444
Author(s):  
Sharad R. Kane

SummaryRadial structure of impulsive hard X-ray and microwave sources in solar flares is not well known at the present time. Measurements of near-the-limb flares with a high spatial and temporal resolution is, of course, the best way to determine the radial structure of these sources. In absence of such measurements, particularly for the hard X-ray emission, behind-the-limb flares provide (through occultation) a means of observing the coronal part of the impulsive source. Here we summarize the characteristics of the impulsive coronal X-ray source deduced from multi-spacecraft observations of a behind-the-limb flare and their implications with respect to impulsive microwave source.


Solar Physics ◽  
1987 ◽  
Vol 111 (1) ◽  
pp. 81-87 ◽  
Author(s):  
Keizo Kai

Author(s):  
V. D. Tereshchenko ◽  
E. B. Vasil'ev ◽  
O. F. Ogloblina ◽  
V. A. Tereshchenko ◽  
S. M. Chernyakov

Author(s):  
Sedeer el-Showk
Keyword(s):  

2003 ◽  
Vol 32 (12) ◽  
pp. 2483-2488
Author(s):  
C GOFF ◽  
S MATTHEWS ◽  
L HARRA
Keyword(s):  

2010 ◽  
Vol 180 (9) ◽  
pp. 997 ◽  
Author(s):  
B.V. Somov

2007 ◽  
Vol 13 (1s) ◽  
pp. 99-100
Author(s):  
V.G. Lozitsky ◽  
Keyword(s):  

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