scholarly journals On the Role of Last Closed Drift Shell Dynamics in Driving Fast Losses and Van Allen Radiation Belt Extinction

2018 ◽  
Vol 123 (5) ◽  
pp. 3692-3703 ◽  
Author(s):  
L. Olifer ◽  
I. R. Mann ◽  
S. K. Morley ◽  
L. G. Ozeke ◽  
D. Choi
2020 ◽  
Vol 125 (9) ◽  
Author(s):  
A. Y. Drozdov ◽  
M. E. Usanova ◽  
M. K. Hudson ◽  
H. J. Allison ◽  
Y. Y. Shprits

2021 ◽  
pp. 85-119
Author(s):  
Hannu E. J. Koskinen ◽  
Emilia K. J. Kilpua

AbstractUnderstanding the role of plasma waves, extending from magnetohydrodynamic (MHD) waves at ultra-low-frequency (ULF) oscillations in the millihertz range to very-low-frequency (VLF) whistler-mode emissions at frequencies of a few kHz, is necessary in studies of sources and losses of radiation belt particles. In order to make this theoretically heavy part of the book accessible to a reader, who is not familiar with wave–particle interactions, we have divided the treatise into three chapters. In the present chapter we introduce the most important wave modes that are critical to the dynamics of radiation belts. The drivers of these waves are discussed in Chap. 10.1007/978-3-030-82167-8_5 and the roles of the wave modes as sources and losses of radiation belt particles are dealt with in Chap. 10.1007/978-3-030-82167-8_6.


2011 ◽  
Vol 116 (A9) ◽  
pp. n/a-n/a ◽  
Author(s):  
A. Y. Ukhorskiy ◽  
M. I. Sitnov ◽  
R. M. Millan ◽  
B. T. Kress

1996 ◽  
Vol 60 (4) ◽  
pp. 639-645
Author(s):  
J.D. Kaplunov ◽  
E.V. Nolde
Keyword(s):  

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