Electron acceleration due to small pulses in shock waves in inhomogeneous plasmas: Perpendicular propagation

2006 ◽  
Vol 13 (6) ◽  
pp. 063110 ◽  
Author(s):  
Masatoshi Sato ◽  
Yukiharu Ohsawa
2002 ◽  
Vol 391 (2) ◽  
pp. 749-756 ◽  
Author(s):  
G. Mann ◽  
H. T. Classen ◽  
E. Keppler ◽  
E. C. Roelof

2005 ◽  
Vol 12 (5) ◽  
pp. 052308 ◽  
Author(s):  
Masatoshi Sato ◽  
Seiji Miyahara ◽  
Yukiharu Ohsawa

1980 ◽  
Vol 4 (1) ◽  
pp. 53-55 ◽  
Author(s):  
R. T. Stewart ◽  
A. Magun

Perhaps the most direct evidence to date for shock wave acceleration of electrons in the solar corona is provided by radio observations of Type II bursts containing herringbone structure (Roberts 1959). On spectral records the herringbones appear to resemble miniature forward and reverse drift Type III bursts extending above and below the Type II backbone.


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