Laboratory Simulation of Thermal Convection in Rotating Planets and Stars-Reference-Cited by-同舟云学术

Laboratory Simulation of Thermal Convection in Rotating Planets and Stars

Published:1976-01-09 Issue:4222 Volume:191 Page:81-83
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Busse F. H.¹,Carrigan C. R.¹

Affiliation:

1. Department of Geophysics and Space Physics, University of California, Los Angeles 90024

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference8 articles.

1. BULLARD, E.C., THE MAGNETIC FIELD WITHIN THE EARTH, PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES 197: 433 (1949).

2. P INT SCH PHYSICS EN 1967

3. BUSSE, F.H., DIFFERENTIAL ROTATION IN STELLAR CONVECTION ZONES .2., ASTRONOMY AND ASTROPHYSICS 28: 27 (1973).

4. BUSSE, F.H., DIFFERENTIAL ROTATION IN STELLAR CONVECTION ZONES, ASTROPHYSICAL JOURNAL 159: 629 (1970).

5. BUSSE, F.H., MODEL OF GEODYNAMO, GEOPHYSICAL JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY 42: 437 (1975).

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