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The lack of chemical separation during the diffusion of gas into solar magnetic tubes

✍ Scribed by R. G. Giovanelli


Publisher
Springer
Year
1979
Tongue
English
Weight
87 KB
Volume
62
Category
Article
ISSN
0038-0938

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✦ Synopsis


At a temperature well above Train, SO that hydrogen is mainly ionized and diffuses negligibly into magnetic tubes, helium can still be mainly neutral so that chemical differentiation could occur. Calculation shows that the rate is too small to acccount for variations in chemical abundance found in the solar wind.


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