Electron Acceleration in Solar Flares by Fast Mode Waves: Quasi‐linear Theory and Pitch‐Angle Scattering

1997 ◽  
Vol 491 (2) ◽  
pp. 939-951 ◽  
Author(s):  
James A. Miller
1998 ◽  
Vol 493 (1) ◽  
pp. 451-459 ◽  
Author(s):  
Geoffrey T. Lenters ◽  
James A. Miller

2001 ◽  
Vol 203 ◽  
pp. 577-579
Author(s):  
M. Vandas

Spacecraft measurements of energetic electrons in the vicinity of the Earth's bow shock and interplanetary shocks are analyzed and compared with theoretical calculations. It is concluded that shock drift acceleration of electrons is very modified by an additional process, probably by strong pitch angle scattering. Calculations including this effect are presented.


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.


1996 ◽  
Vol 461 ◽  
pp. 445 ◽  
Author(s):  
James A. Miller ◽  
T. N. Larosa ◽  
R. L. Moore

1999 ◽  
Vol 518 (2) ◽  
pp. 974-984 ◽  
Author(s):  
B. R. Ragot
Keyword(s):  

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