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Seismology of the Sun and the Distant Stars
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Seismology of the Sun and the Distant Stars

There is now good reason to suppose that a sufficiently careful analysis will lead to a direct determination of the helium abundance in the solar convection zone, especially when foreseeable further improvements in the observations have been achieved.
Redaktør
D.O. Gough
Opplag
Softcover reprint of the original 1st ed. 1986
ISBN
9789401085472
Språk
Engelsk
Vekt
310 gram
Utgivelsesdato
13.10.2011
Forlag
Springer
Antall sider
492