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Problems of Solar and Stellar Oscillations
Tallenna

Problems of Solar and Stellar Oscillations

In the last few years we have become aware that the frequencies of the five-minute modes of high degree, which constitute the major component of the oscillations discovered twenty years ago by Evans and Michaud, can be used to put quite tight bounds on the stratification of the solar convection zone.
Alaotsikko
Proceedings of the 66th IAU Colloquium held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981
Toimittaja
D.O. Gough
Painos
Softcover reprint of the original 1st ed. 1983
ISBN
9789400970908
Kieli
englanti
Paino
310 grammaa
Julkaisupäivä
28.10.2011
Kustantaja
Springer
Sivumäärä
494