On the discreteness of the spectrum of scales of motion in the solar convection zone

Details On the discreteness of the spectrum of scales of motion in the solar convection zone On the discreteness of the spectrum of scales of motion in the solar convection zone

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978azh....55..404s&link_type=abstract

Astronomicheskii Zhurnal, vol. 55, Mar.-Apr. 1978, p. 404-410. In Russian.

Astronomy and Astrophysics

Astronomy

Atmospheric Models, Benard Cells, Convection, Solar Atmosphere, Atmospheric Circulation, Heuristic Methods

Scientific paper

The new heuristic approach to the calculation of characteristic scales of motion in the solar convection zone is suggested. It is shown that cell convection is inevitable and more beneficial energetically. As a consequence, the meridional circulation and differential rotation must be functions of longitude, latitude and time. The largest and the smallest scales of motion are discussed briefly.

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