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Geomagnetic activity driven by solar wind turbulence

✍ Scribed by R. D’Amicis; R. Bruno; B. Bavassano


Publisher
Elsevier Science
Year
2010
Tongue
English
Weight
461 KB
Volume
46
Category
Article
ISSN
0273-1177

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Solar wind heating by heat conduction dr
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Nonlinear saturation of the ion acoustic instability, driven by finite heat conduction in the solar wind, via resonance broadening is considered. The calculations based on the Hartle and Sturrock model show that this process can heat ions faster than the electrons, thereby, leading to the reduction