Possible detection of Jovian global oscillations

Details Possible detection of Jovian global oscillations Possible detection of Jovian global oscillations

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248..281s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 1, Aug. 1991, p. 281-291.

Astronomy and Astrophysics

Astrophysics

37

Jupiter (Planet), Planetary Structure, Power Spectra, Seismology, Spherical Harmonics, Astronomical Spectroscopy, Telescopes

Scientific paper

Observations of the Jupiter were carried out using a refined version of the stellar seismometer with a sensitivity of better than 50 cm/s. The observations revealed the existence of strong velocity variations of the planets in the 10-20-min period range. It is concluded that the observed variations can only be explained as global acoustic modes. The frequencies of the modes are examined with reference to the internal structure of the planet.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1724351