Modeling of frontal cloudiness in the atmospheres of giant planets. I - Calculation method

Details Modeling of frontal cloudiness in the atmospheres of giant planets. I - Calculation method Modeling of frontal cloudiness in the atmospheres of giant planets. I - Calculation method

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...15i&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 2, Mar.-Apr. 1992, p. 15-24, 35. In Russian.

Computer Science

Atmospheric Models, Cloud Cover, Diffusion Coefficient, Gas Giant Planets, Planetary Atmospheres, Wind Velocity, Ammonia, Dynamic Models, Jupiter (Planet), Water

Scientific paper

A system of equations is considered which describes the formation and evolution of two-component frontal cloud systems in the atmospheres of giant planets. It is assumed that horizontal motions of atmospheric masses are absent at the region boundary and that within the region velocities vary in accordance with a parabolic law. For such a simple dynamic model, the three-dimensional distribution of moisture and ammonia contents is calculated for the Jovian atmosphere.

Affiliated with

Also associated with

No associations

Rating

Modeling of frontal cloudiness in the atmospheres of giant planets. I - Calculation method 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 Modeling of frontal cloudiness in the atmospheres of giant planets. I - Calculation method, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling of frontal cloudiness in the atmospheres of giant planets. I - Calculation method will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1738383