> From a.cidadao@mail.telepac.pt Fri Mar  1 05:44 MST 2002
X-Sender: cidadao@mail.telepac.pt
Date: Fri, 01 Mar 2002 12:36:45 +0000
From: Antonio Cidadao <a.cidadao@mail.telepac.pt>
Subject: Jupiter data, Feb 26 and 27

Hi all,

Here are my latest images, and I'm currently processing the other Feb data.

The SEdisturbance is seen in the Feb26 images, perhaps now less conspicuous
on the CH4 band. The methane dark STB segments continue to be present, and
the NNTB oval is still methane bright.

The feb 27 images show the GRS, BA and SSTC Wos, NEB with B4 and the
extensive rift system (a mid-NEB barge / white spot is seen). The GRS and
BA in methane-band continue to present the morphology described in earlier
messages. A few CH4-bright clouds are seen in SEB following the GRS.

In clear and RGB images, a smal dark spot is seen immediately N of the GRS.

It is always impressive to see that even large /dark barges like B4 are
virtually invisible in IR.

Good observations

Antonio 


> From sherrodc@ipa.net Fri Mar  1 06:34 MST 2002
From: "Clay Sherrod" <sherrodc@ipa.net>
Subject: Re: Jupiter data, Feb 26 and 27
Date: Fri, 1 Mar 2002 07:32:50 -0600

Good morning Antonio -
Your RGB image of Feb. is particularly impressive and of course useful to
study the area immediately surrounding the GRS and BA interaction and I note
the very fine detail of activity in the following wake of these two.
Likewise, the significant rift leading up to B-4 is incredible and your
images are really helping to define its [the rift, not B-4] "renewed"
development after appearing to wane recently.

I look forward to others as you work your way through February....your care
in processing so carefully each wavelength is greatly appreciated.

Clay
----------------------------------------
Dr. P. Clay Sherrod
sherrodc@ipa.net
Arkansas Sky Observatory
www.arksky.org