A new method for registration of oscillations in atmospheres of Jovian planets

Details A new method for registration of oscillations in atmospheres of Jovian planets A new method for registration of oscillations in atmospheres of Jovian planets

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..206v&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 206-208

Physics

Scientific paper

Our analysis shows that a change of gas and aerosol vertical speed in the range of w=(10-50) cm/s determines the volume of top layers of visible clouds of giant planets, and therefore, may allow to find the reflectance characteristics of an observable cloud layer. In the presence of the certain factors, causing a change of a value of an air vertical moving speed as well as direction of such moving, it will modulate processes of cloudy formation and/or their destruction. In this connection we assume that the fluctuation processes of cloudy creation and their disintegration can serve as a preferable method for registration of possible giant planetary atmosphere oscillations.

Affiliated with

Also associated with

No associations

Rating

A new method for registration of oscillations in atmospheres of Jovian planets 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 A new method for registration of oscillations in atmospheres of Jovian planets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A new method for registration of oscillations in atmospheres of Jovian planets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1386788