Excitation mechanism of very slow oscillations of the Jovian atmosphere

Details Excitation mechanism of very slow oscillations of the Jovian atmosphere Excitation mechanism of very slow oscillations of the Jovian atmosphere

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...359l..29l&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 359, Aug. 10, 1990, p. L29-L32.

Astronomy and Astrophysics

Astrophysics

6

Gravity Waves, Jupiter Atmosphere, Planetary Rotation, Wave Excitation, Low Frequencies, Phase Velocity, Stellar Oscillations

Scientific paper

An excitation mechanism is proposed for the recently discovered very slow wavelike structure in the Jovian atmosphere, which is regarded as normal mode gravity-wave oscillations of this atmosphere. Such oscillations are excited through resonance couplings with prograde inertial oscillations of the convective interior having negative energies. The amplitude of a low-frequency oscillation of the Jovian atmosphere can be large only in the equatorial region.

Affiliated with

Also associated with

No associations

Rating

Excitation mechanism of very slow oscillations of the Jovian atmosphere 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 Excitation mechanism of very slow oscillations of the Jovian atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Excitation mechanism of very slow oscillations of the Jovian atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1125755