Variability of low-energy ion flux profiles on interplanetary shock fronts

2006 ◽  
Vol 111 (A12) ◽  
Author(s):  
M. Neugebauer ◽  
J. Giacalone ◽  
E. Chollet ◽  
D. Lario
1984 ◽  
Vol 4 (2-3) ◽  
pp. 331-334 ◽  
Author(s):  
E.I. Morozova ◽  
N.F. Pissarenko ◽  
W. Riedler ◽  
K. Schwingenschuh ◽  
G. Schelch ◽  
...  

2017 ◽  
Vol 55 (1) ◽  
pp. 30-45 ◽  
Author(s):  
V. G. Eselevich ◽  
N. L. Borodkova ◽  
M. V. Eselevich ◽  
G. N. Zastenker ◽  
Y. Šafránkova ◽  
...  

1988 ◽  
Vol 101 ◽  
pp. 309-324
Author(s):  
R.D. Blandford

AbstractSome recent developments in the theory of particle acceleration at supernova shock fronts are reviewed and the confrontation of this theory with measurements of galactic cosmic rays and observations of supernova remnants is discussed. Supernova shock waves are able to account for the energetics, spectrum and composition of galactic cosmic rays, though it remains difficult to understand acceleration of ∼ 105 GeV particles. Recent developments in the analysis of interplanetary shock waves and in the numerical simulation of quasi-parallel shocks are encouraging. Interpretations of different categories of remnants are reviewed and a speculative interpretation of the optical companion to SN1987a is discussed.


2008 ◽  
Vol 79 (2) ◽  
pp. 02B719 ◽  
Author(s):  
A. V. Vizir ◽  
M. V. Shandrikov ◽  
E. M. Oks
Keyword(s):  
Ion Flux ◽  

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