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The Solar Hydrogen Convection Zone and its Direct Influence on the Photosphere

Published online by Cambridge University Press:  16 November 2021

E. A. Spiegel
E. A. Spiegel*
Affiliation:
Physics Department, New York University

Extract

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The discovery of oscillatory motion in the solar photosphere and of the ‘super-granulation’ in the chromosphere has changed our ideas about the hydrodynamics of the solar atmosphere considerably. In this Joint Discussion we shall mainly consider the theoretical implications of this change. As the ultimate aim is an understanding of the hydrodynamics in all stellar atmospheres—not only in the Sun, some discussion of other stellar atmospheres will be included.

Type
Part 4 Joint Discussions
Information
Transactions of the International Astronomical Union , Volume 12 , Issue 2 , 1966 , pp. 539 - 542
Copyright
Copyright © Academic Press 1966 

References

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