Substorm injection of relativistic electrons to geosynchronous orbit during the great magnetic storm of March 24, 1991

2001 ◽  
Vol 106 (A11) ◽  
pp. 25759-25776 ◽  
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J. C. Ingraham ◽  
T. E. Cayton ◽  
R. D. Belian ◽  
R. A. Christensen ◽  
R. H. W. Friedel ◽  
...  
2003 ◽  
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E.A. Ginzburg ◽  
N.N. Pavlov ◽  
P.M. Svidsky

2001 ◽  
Vol 106 (A12) ◽  
pp. 30039-30046 ◽  
Author(s):  
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Richard A. Goldberg ◽  
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E. E. Gaines ◽  
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2009 ◽  
Vol 36 (1) ◽  
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Y. Kasahara ◽  
Y. Miyoshi ◽  
Y. Omura ◽  
O. P. Verkhoglyadova ◽  
I. Nagano ◽  
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2013 ◽  
Vol 56 (5) ◽  
pp. 532-545
Author(s):  
ZHANG Xiao-Fang ◽  
LIU Jun ◽  
WU Yao-Ping ◽  
ZHOU Lü ◽  
LIU Song-Tao

2003 ◽  
Vol 31 (4) ◽  
pp. 1059-1062
Author(s):  
W.Dean Pesnell ◽  
Richard A. Goldberg ◽  
D.L. Chenette ◽  
M. Schulz ◽  
E.E. Gaines

1989 ◽  
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pp. 1129-1132 ◽  
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D. L. Chenette ◽  
D. N. Baker ◽  
D. Moses

Space Weather ◽  
2011 ◽  
Vol 9 (6) ◽  
pp. n/a-n/a ◽  
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X. Li ◽  
E. Burin des Roziers ◽  
S. Monk

2008 ◽  
Vol 4 (S257) ◽  
pp. 457-463
Author(s):  
Ilan Roth

AbstractIn situ and remote observations indicate that relativistic or ultra relativistic electrons are formed at various magnetized configurations. It is suggested that a specific bootstrap mechanism operates in some of these environments. The mechanism applies to (a) relativistic electrons observed on localized field lines in outer radiation belt - through a process initiated at a distant substorm injection; (b) relativistic electrons observed at the interplanetary medium - through a process initiated via coronal injection, at large distances from flares or propagating CME; (c) ultra-relativistic electrons deduced at the galactic jets - through a process initiated via local injection at the small-scale magnetic field. The injected nonisotropic electrons excite whistler waves which boost efficiently the tail of the electron distribution.


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