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

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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.
Redaktör
D.O. Gough
Upplaga
Softcover reprint of the original 1st ed. 1986
ISBN
9789401085472
Språk
Engelska
Vikt
310 gram
Utgivningsdatum
2011-10-13
Förlag
Springer
Sidor
492