|
IJW / Laboratory
and Theory Discipline
Observer seeks
modeling assistance:
From tejf@hotmail.com
Thu Jan 14 13:24 CST 1999
We have obtained
during last years many good data about the latitudinal variations of the
limb darkening and the
methane absorption bands intensity (equivalent widths and central residual
intensity) for disks of Jupiter and Saturn using CCD-camera ST-6V and
1-meter telescope of our observatory Assy at 2750 m altitude (about 100
km eastern Alma-Ata city). I would like to ask you if possible to connect
me kindly with any theoretician who may be interested in the interpretation
of these data in terms of multilayer cloud atmospheric radiative transfer
model (we haven't that opportunity here). I hope it would be good joint
work. If you will find an opportunity and time to look on our observatory
and some pictures illustrating our planetary studies, please, find in
Internet URL
http://members.tripod.com/~Planlab/index.html
and also some hyperreferences there about Jupiter spectrophotometry. There
are some graphs about the methane absorption distribution on Jupiter's
disk.
With kind regards,
Victor Tejfel
Prof., Head of Laboratory of Lunar and Planetary Physics,
Fessenkov Astrophysical Institute,
Alma-Ata, Kazakhstan
e-mail: tejf@hotmail.com
tejf@afi.academ.alma-ata.su
For questions, comments,
or to be added to the subscription list, please notify:
Julianne I. Moses
Lunar and Planetary Institute
3600 Bay Area Blvd.
Houston, TX 77058-1113
moses@lpi.usra.edu
February 1, 1999
|