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Solar wind induction in Mercury: Constraints on the formation of a magnetosphere

โœ Scribed by F. Herbert; M. Wiskerchen; C.P. Sonett; J.K. Chao


Book ID
107765264
Publisher
Elsevier Science
Year
1976
Tongue
English
Weight
1020 KB
Volume
28
Category
Article
ISSN
0019-1035

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The abundance of3He in the solar wind -
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3He is an intermediate product in the proton-proton chain, and standard models of the Sun predict a large bulge of enhanced 3He abundance near Mr/M o = 0.6 in the contemporary Sun. The relatively low abundance of 3He at the solar surface, which is derived from solar wind observations, poses severe c