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

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

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...62...51g&link_type=abstract

Solar Physics, vol. 62, May 1979, p. 51, 52.

Physics

Gas Flow, Magnetic Diffusion, Neutral Gases, Solar Magnetic Field, Solar Wind, Thermal Diffusion, Chemical Reactions, Gas Density, Gas Pressure, Helium Atoms, Hydrogen Atoms, Ionized Gases, Solar Physics

Scientific paper

At a temperature well above minimum, 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 account for variations in chemical
abundance found in the solar wind.

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