Astron. Astrophys. 327, 1253-1261 (1997)
The 1993 south equatorial belt revival and other features
in the Jovian atmosphere: an observational perspective
F. Moreno 1,
A. Molina 1, 2 and
J.L. Ortiz 1
1 Instituto de Astrofísica de Andalucía,
CSIC, PO Box 3004, E-18080 Granada, Spain
2 Departamento de
F sica Aplicada, Universidad de
Granada, Spain
Received 20 May 1997 / Accepted 21 July 1997
Abstract
An excellent-quality set of images of the 1993 Jovian South
Equatorial Belt (SEB) revival are shown and discussed. For the first
time, this major SEB event was recorded since the very early stages of
its development to its end at a variety of wavelengths from the
ultraviolet to the near-infrared region of the spectrum. Our analysis
supports, at least for the locus B, the Reese theory of the presence
of three sources uniformly rotating with respect to System III from
which the SEB disturbances develop. Other Jovian features were also
present in these images, such as the activity in the South Temperate
Belt or the presence of the so-called methane spots, which are shown
to be photometrically analogous to the Great Red Spot on Jupiter. A
general characterization of all the Jovian regions at the time of the
South Equatorial Belt disturbance is done by computing the limb
darkening coefficients as a function of latitude and wavelength. This
provides a useful reference to compare with other future measurements.
The limb darkening coefficient at the brightest spot associated to the
SEB event in April shows a different behaviour in its wavelength
dependence as compared to all the other Jovian regions, a result that
would imply a different particle loading and/or particle size
distribution in those regions as a consequence of vigorous
dynamics.
Key words: planets and satellites: individual: Jupiter
Send offprint requests to: F. Moreno, e-mail: fernando@iaa.es
Contents
© European Southern Observatory (ESO) 1997
Online publication: April 6, 1998
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