Heat transfer by a meridional circulation cell and the static stability of the atmosphere of a slowly rotating planet.

Details Heat transfer by a meridional circulation cell and the static stability of the atmosphere of a slowly rotating planet. Heat transfer by a meridional circulation cell and the static stability of the atmosphere of a slowly rotating planet.

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cosre..27..797z&link_type=abstract

Cosmic Res., Vol. 27, No. 6, p. 797 - 806

Other

Venus Atmosphere

Scientific paper

Equations are derived for the determination of the equatorial-polar temperature difference and the static stability parameter in the atmosphere of a planet for which the principal heat transfer mechanism is ordered meridional circulation. The spherical geometry of the planetary atmosphere is taken into account, and the flow in the cell is specified in general form, in contrast to the a priori approximation by Stone, who was first to apply such an approach. The obtained results are investigated to evaluate the periods of thermal adaptation of the atmosphere, the scale of the wind velocity, and other characteristics of atmospheric circulation on Venus.

Affiliated with

Also associated with

No associations

Rating

Heat transfer by a meridional circulation cell and the static stability of the atmosphere of a slowly rotating planet. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Heat transfer by a meridional circulation cell and the static stability of the atmosphere of a slowly rotating planet., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Heat transfer by a meridional circulation cell and the static stability of the atmosphere of a slowly rotating planet. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-780277