Stability of the solar wind against the whistler mode
1978 ◽
Vol 20
(2)
◽
pp. 225-230
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Keyword(s):
The Sun
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The stability of the solar wind against the whistler mode is analyzed. It is shown that the solar wind can become unstable owing to this mode after a distance of 100 R from the sun. The minimum value of the relative velocity (Ur) between ∝-particles and protons for the excitation of this instability is the proton thermal velocity αi. The maximum growth rate at 200 R occurs for the values of the parameters kρi = 0·3,(T┤/T∥)i = 0·3 and Ur/αi = 0·5.
Keyword(s):
2008 ◽
Vol 38
(4)
◽
pp. 840-861
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Keyword(s):
Keyword(s):
1975 ◽
Vol 14
(1)
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pp. 143-152
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Keyword(s):
Keyword(s):
Keyword(s):
1992 ◽
Vol 25
(6)
◽
pp. 167-183
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1977 ◽
Vol 52
(2)
◽
pp. 113-117
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1987 ◽
Vol 44
(11)
◽
pp. 1995-2001
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2012 ◽
Vol 57
(2)
◽
pp. 554-566
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Keyword(s):