Evidence for >30-keV Electrons Accelerated in the Shock Transition Region Beyond the Earth's Magnetospheric Boundary

1964 ◽  
Vol 13 (5) ◽  
pp. 149-152 ◽  
Author(s):  
C. Y. Fan ◽  
G. Gloeckler ◽  
J. A. Simpson
2003 ◽  
Vol 10 (4) ◽  
pp. 1113-1119 ◽  
Author(s):  
Nobue Shimada ◽  
Masahiro Hoshino

1998 ◽  
Vol 25 (15) ◽  
pp. 2929-2932 ◽  
Author(s):  
S. D. Bale ◽  
P. J. Kellogg ◽  
D. E. Larsen ◽  
R. P. Lin ◽  
K. Goetz ◽  
...  

2019 ◽  
Vol 46 (2) ◽  
pp. 562-570 ◽  
Author(s):  
Shan Wang ◽  
Li‐Jen Chen ◽  
Naoki Bessho ◽  
Michael Hesse ◽  
Lynn B. Wilson ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 315-321 ◽  
Author(s):  
M. G. Rovira ◽  
J. M. Fontenla ◽  
J.-C. Vial ◽  
P. Gouttebroze

AbstractWe have improved previous model calculations of the prominence-corona transition region including the effect of the ambipolar diffusion in the statistical equilibrium and energy balance equations. We show its influence on the different parameters that characterize the resulting prominence theoretical structure. We take into account the effect of the partial frequency redistribution (PRD) in the line profiles and total intensities calculations.


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