The Temperature of the Bright Knots at the Tops of Solar Flare Loops

1996 ◽  
Vol 459 ◽  
pp. 773 ◽  
Author(s):  
G. A. Doschek ◽  
U. Feldman
Keyword(s):  
1999 ◽  
Vol 527 (2) ◽  
pp. 945-957 ◽  
Author(s):  
Vahe Petrosian ◽  
Timothy Q. Donaghy

Solar Physics ◽  
2010 ◽  
Vol 263 (1-2) ◽  
pp. 163-174 ◽  
Author(s):  
I. V. Zimovets ◽  
A. B. Struminsky

2016 ◽  
Vol 823 (1) ◽  
pp. L16 ◽  
Author(s):  
Hui Tian ◽  
Peter R. Young ◽  
Katharine K. Reeves ◽  
Tongjiang Wang ◽  
Patrick Antolin ◽  
...  

1997 ◽  
Vol 487 (2) ◽  
pp. 936-955 ◽  
Author(s):  
Markus J. Aschwanden ◽  
Robert M. Bynum ◽  
Takeo Kosugi ◽  
Hugh S. Hudson ◽  
Richard A. Schwartz

2004 ◽  
Vol 614 (2) ◽  
pp. 1022-1027 ◽  
Author(s):  
S. Patsourakos ◽  
S. K. Antiochos ◽  
J. A. Klimchuk

2012 ◽  
Vol 8 (S294) ◽  
pp. 153-154
Author(s):  
Jing Huang

AbstractFrom the observations of radio and HXR bursts, the escape rate of energetic electrons trapped in the flare loops is studied based on the trap-plus-precipitation model for the kinematics of energetic electrons in solar flares. Coulomb collision is regarded as the main pitch angle scattering of trapped electrons in the decay phase of the event on 2004 December 1. The escape rate of trapped electrons decreases firstly and then increases, which indicates the evolution of the plasma density in the flare loops during the decay phase.


1983 ◽  
Author(s):  
E. J. Schmahl ◽  
M. R. Kundu ◽  
P. B. Landecker ◽  
D. L. McKenzie
Keyword(s):  
X Rays ◽  

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