The 90-day oscillation of the jovian Great Red SPOT

Details The 90-day oscillation of the jovian Great Red SPOT The 90-day oscillation of the jovian Great Red SPOT

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jbaa..106...40h&link_type=abstract

Journal of the British Astronomical Association, vol.106, no.1, p.40-43

Astronomy and Astrophysics

Astronomy

Jupiter, Great Red Spot

Scientific paper

The purpose of this contribution is to study the possible existence of
the 90-day longitude oscillation of Jupiter's Great Red Spot (GRS) which
had been discovered in the 1960s over long time intervals. Additionally,
further possible periodicities in the longitudinal motion of the GRS in
the 40 to 400 day range are considered.

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