PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2007-07-31 NOTE = " E-mail and other messages concerning MGS Radio Science on or about 2007/005." END_OBJECT = TEXT END From sami.asmar@jpl.nasa.gov Fri Jan 5 22:33:05 2007 Return-Path: Received: from nmta1.jpl.nasa.gov (nmta1.jpl.nasa.gov [137.78.160.214]) by magellan.stanford.edu (8.11.7p2+Sun/8.11.7) with ESMTP id l066X5a19856 for ; Fri, 5 Jan 2007 22:33:05 -0800 (PST) Received: from xmta2.jpl.nasa.gov (xmta2.jpl.nasa.gov [137.78.160.56]) by nmta1.jpl.nasa.gov (Switch-3.1.9/Switch-3.1.9) with ESMTP id l066X0IE029963; Fri, 5 Jan 2007 22:33:00 -0800 Received: from SAMI.jpl.nasa.gov (vpn-149-246-051.jpl.nasa.gov [128.149.246.51]) by xmta2.jpl.nasa.gov (Switch-3.1.9/Switch-3.1.9) with ESMTP id l066WwXn001144; Fri, 5 Jan 2007 22:32:59 -0800 Message-Id: <6.2.1.2.2.20070105222824.02faebf0@mail.jpl.nasa.gov> X-Mailer: QUALCOMM Windows Eudora Version 6.2.1.2 Date: Fri, 05 Jan 2007 22:29:38 -0800 To: Daniel.S.Kahan@jpl.nasa.gov, Aseel.Anabtawi@jpl.nasa.gov, dhinson@stanford.edu, rsimpson@magellan.stanford.edu, len.tyler@stanford.edu From: Sami Asmar Subject: MEX MGS Mime-Version: 1.0 Content-Type: text/plain; charset="us-ascii"; format=flowed X-Source-IP: vpn-149-246-051.jpl.nasa.gov [128.149.246.51] X-Source-Sender: sami.asmar@jpl.nasa.gov X-AUTH: Authorized Content-Length: 762 Status: RO >>- The second MGS imaging data are still being studied by the imaging >>team. According to Alan Moorhouse (previous deputy SOM for MEX), they >>found "something" in one channel but need more analysis to make >>conclusive answer. There is no information on when the final results will >>be available. >> >>- Tom Thorpe and Pat Esposito once again thanked MEX team for their extra >>effort. Tom said the MGS project is winding down. Commanding and tracking >>of MGS will end by end of January along with most of the operations >>except for the archiving process which will continue until May. >> >>- Pat Esposito said MGS Nav team is still working on a long term >>prediction of MGS orbit and any finding from the MEX imaging will be very >>helpful.