Spatial structure of greater than 100 keV X-ray sources in solar flares

1982 ◽  
Vol 254 ◽  
pp. L53 ◽  
Author(s):  
S. R. Kane ◽  
E. E. Fenimore ◽  
R. W. Klebesadel ◽  
J. G. Laros
Keyword(s):  
Solar Physics ◽  
1987 ◽  
Vol 107 (2) ◽  
pp. 263-269 ◽  
Author(s):  
A. Gordon Emslie ◽  
Marcos E. Machado

1986 ◽  
Vol 6 (6) ◽  
pp. 139-142
Author(s):  
A.G. Emslie ◽  
J.A. Fennelly ◽  
M.E. Machado

X -ray and ultraviolet observations of flares have provided much important information on their spatial structure and magnetic topology. The early observations from Skylab emphasized the role of simple loops and loop arcades, but later observations from the Solar Maximum Mission have greatly complicated this picture. Flares appear in a multitude of loops with complex spatial and temporal interrelations. In many cases, interactions between different loops appear to play a crucial role. The inferred magnetic topology of solar flares will be reviewed with emphasis on the implications for processes of energy release and transfer. It will be shown that the spatial resolution of the observations obtained so far is still inadequate for solving many basic questions of solar flare research.


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

2021 ◽  
Vol 366 (1) ◽  
Author(s):  
Bo Xiong ◽  
Ting Wang ◽  
Xiaolin Li ◽  
Yunxing Yin

Solar Physics ◽  
1986 ◽  
Vol 105 (1) ◽  
pp. 87-99 ◽  
Author(s):  
E. J. Schmahl ◽  
M. R. Kundu ◽  
F. T. Erskine
Keyword(s):  
X Ray ◽  

1988 ◽  
Vol 148 (1) ◽  
pp. 75-84 ◽  
Author(s):  
Ranjna Bakaya ◽  
R. R. Rausaria ◽  
P. N. Khosa
Keyword(s):  

2013 ◽  
Vol 13 (12) ◽  
pp. 1482-1492 ◽  
Author(s):  
You-Ping Li ◽  
Wei-Qun Gan ◽  
Li Feng ◽  
Si-Ming Liu ◽  
A. Struminsky

Sign in / Sign up

Export Citation Format

Share Document