Identification of Ion-Cyclotron Drift Instability with Discrete and Continuous Spectra

1974 ◽  
Vol 33 (18) ◽  
pp. 1076-1079 ◽  
Author(s):  
H. W. Hendel ◽  
M. Yamada
1977 ◽  
Vol 60 (3) ◽  
pp. 199-202 ◽  
Author(s):  
T. Maekawa ◽  
M. Sando ◽  
S. Tanaka

1971 ◽  
Vol 11 (4) ◽  
pp. 323-327 ◽  
Author(s):  
A.B. Mikhailovsky

Physics ◽  
2021 ◽  
Vol 3 (4) ◽  
pp. 1175-1189
Author(s):  
Shaaban M. Shaaban ◽  
Marian Lazar ◽  
Peter H. Yoon ◽  
Stefaan Poedts ◽  
Rodrigo A. López

The ability of space plasmas to self-regulate through mechanisms involving self-generated fluctuations is a topic of high interest. This paper presents the results of a new advanced quasilinear (QL) approach for the instability of electromagnetic ion-cyclotron modes driven by the relative alpha-proton drift observed in solar wind. For an extended parametric analysis, the present QL approach includes also the effects of intrinsic anisotropic temperatures of these populations. The enhanced fluctuations contribute to an exchange of energy between proton and alpha particles, leading to important variations of the anisotropies, the proton-alpha drift and the temperature contrast. The results presented here can help understand the observational data, in particular, those revealing the local variations associated with the properties of protons and alpha particles as well as the spatial profiles in the expanding solar wind.


1979 ◽  
Vol 22 (9) ◽  
pp. 1764 ◽  
Author(s):  
S. Peter Gary ◽  
R. A. Gerwin

1976 ◽  
Vol 37 (C5) ◽  
pp. C5-233-C5-235
Author(s):  
G. N. Flerov
Keyword(s):  

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