Microphysical properties of two-component stratified cloud cover in the atmospheres of the giant planets. I - A calculation method. Jupiter

Details Microphysical properties of two-component stratified cloud cover in the atmospheres of the giant planets. I - A calculation method. Jupiter Microphysical properties of two-component stratified cloud cover in the atmospheres of the giant planets. I - A calculation method. Jupiter

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...22i&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, Mar.-Apr. 1988, p. 22-28. In Russian.

Physics

Atmospheric Stratification, Atmospheric Temperature, Cloud Cover, Jupiter Atmosphere, Adiabatic Conditions, Atmospheric Models, Turbulent Mixing

Scientific paper

A system of equations describing cloud formation and evolution in the atmospheres of the giant planets of Jupiter is presented with allowance for cloud microstructure. The adiabatic model of the atmosphere with an initial temperature of 300 K and an adiabatic gradient of 2.25 K/km is used in the calculations. A relationship is established between atmospheric parameters and the cloud cover characteristics (ammonia content, water content, particle concentration, and the mean radius of particles).

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