Momentum and energy transport in the Sun's convection zone under the observational constraint of flux and temperature homogeneity at the surface
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/BF00152343.pdf
Reference5 articles.
1. Belvedere, G. and Patern�, L.: 1977, Solar Phys. 54, 289.
2. Durney, B. R.: 1976, in V. Bumba and J. Kleczek (eds.), ?Basic Mechanisms of Solar Activity?, IAU Symp. 71, 243.
3. Parker, E. N.: 1975, Astrophys. J. 198, 205.
4. Stix, M.: 1976a, in V. Bumba and J. Kleczek (eds.), ?Basic Mechanisms of Solar Activity?, IAU Symp. 71, 367.
5. Stix, M.: 1976b, Astron. Astrophys. 47, 243.
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1. The Pattern of Large-Scale Convection in the Sun;Secular Solar and Geomagnetic Variations in the Last 10,000 Years;1988
2. The Solar Dynamo: Observations and Theories of Solar Convection, Global Circulation, and Magnetic Fields;Physics of the Sun;1986
3. Compressible convection in a rotating spherical shell. V - Induced differential rotation and meridional circulation;The Astrophysical Journal;1982-05
4. The Present Status of Dynamo Theory;Annual Review of Astronomy and Astrophysics;1981-09
5. Global Circulation of the Sun: Where are we and where are we going?;Highlights of Astronomy;1980
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