PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2007-07-27 NOTE = " E-mail and other messages concerning MGS Radio Science on or about 1998/049." END_OBJECT = TEXT END From hinson@nimbus.Stanford.EDU Tue Feb 17 12:57:49 1998 Received: from nimbus.Stanford.EDU (nimbus.Stanford.EDU [36.10.0.96]) by magellan.Stanford.EDU (8.8.5/8.8.3) with ESMTP id MAA14531 for ; Tue, 17 Feb 1998 12:57:48 -0800 (PST) Received: (from hinson@localhost) by nimbus.Stanford.EDU (8.8.4/8.8.3) id MAA28512; Tue, 17 Feb 1998 12:57:42 -0800 (PST) Date: Tue, 17 Feb 1998 12:57:42 -0800 (PST) From: Dave Hinson Message-Id: <199802172057.MAA28512@nimbus.Stanford.EDU> To: joe@neptune.Stanford.EDU, rsimpson@magellan.Stanford.EDU, trish@rodan.jpl.nasa.gov, len@nova.Stanford.EDU Subject: AAG meeting X-Sun-Charset: US-ASCII Content-Length: 423 Status: RO I phoned in to the AAG (atmospheric advisory group) meeting this morning at 11:30 am. Due to good work by everyone involved, I was able to report results from occultation #31, which had occurred only about 10 hours earlier. TES will be turned off tomorrow and an important source of atmospheric monitoring will be lost. For the next 4-5 weeks, the AAG is very interested in what the radio occultations reveal. -------------------------------------------------------------------- From Paula.M.Eshe@jpl.nasa.gov Tue Feb 17 18:30:02 1998 Received: from eis-msg-012.jpl.nasa.gov (eis-msg-012.jpl.nasa.gov [137.78.18.32]) by magellan.Stanford.EDU (8.8.5/8.8.3) with ESMTP id SAA18139 for ; Tue, 17 Feb 1998 18:30:00 -0800 (PST) Received: from jpl-mhs.jpl.nasa.gov by eis-msg-012.jpl.nasa.gov (X.400 to RFC822 Gateway); Tue, 17 Feb 1998 18:29:57 -0800 X400-Received: by mta Proteus in /c=us/admd=telemail/prmd=nasa/; Relayed; 17 Feb 1998 18:29:55 -0800 X400-Received: by /c=us/admd=telemail/prmd=nasa/; Relayed; 17 Feb 1998 18:29:55 -0800 X400-MTS-Identifier: [/c=us/admd=telemail/prmd=nasa/; 02EF434EA47A3079-Proteus] Content-Identifier: 02EF434EA47A3079 Content-Return: Allowed X400-Content-Type: P2-1988 ( 22 ) Conversion: Allowed Original-Encoded-Information-Types: IA5-Text Priority: normal Disclose-Recipients: Prohibited Alternate-Recipient: Allowed X400-Originator: Paula.M.Eshe@jpl.nasa.gov X400-Recipients: non-disclosure; Message-Id: <02EF434EA47A3079*/c=us/admd=telemail/prmd=nasa/o=jpl/ou=ccmail/s=Eshe/g=Paula/i=M/@MHS> Date: 17 Feb 1998 18:29:55 -0800 From: Paula M Eshe To: len@nova.Stanford.EDU (IPM Return requested), hinson@nimbus.Stanford.EDU (IPM Return requested), joe@neptune.Stanford.EDU (IPM Return requested), rsimpson@magellan.stanford.edu (IPM Return requested), Sami W Asmar (IPM Return requested), Jennifer L Caetta (IPM Return requested), Patricia Priest (IPM Return requested), Salvatore F Abbate (IPM Return requested) Subject: Occultation # 32 MIME-Version: 1.0 Content-Length: 395 Status: O Hello Everything went well at DSS 45 for occultation #32. Record time: 049/02:12:00 to 049/02:26:00 One-way time: 049/02:12:37 to 049/02:25:31 Expected Surface: 049/02:23:32 SPK: spk_i_980216_OD135_145_V1 SOE: p136a.01.soe Script: 98049.45.a135.scr Three attenuation changes, the last one at 02:15:37. The next occultation occurs at 10:35 AM PST Wednesday at DSS 25. Paula ------------------------------------------------------------------ From Paula.M.Eshe@jpl.nasa.gov Wed Feb 18 11:14:56 1998 Received: from eis-msg-012.jpl.nasa.gov (eis-msg-012.jpl.nasa.gov [137.78.18.32]) by magellan.Stanford.EDU (8.8.5/8.8.3) with ESMTP id LAA25030 for ; Wed, 18 Feb 1998 11:14:55 -0800 (PST) Received: from jpl-mhs.jpl.nasa.gov by eis-msg-012.jpl.nasa.gov (X.400 to RFC822 Gateway); Wed, 18 Feb 1998 11:14:17 -0800 X400-Received: by mta Proteus in /c=us/admd=telemail/prmd=nasa/; Relayed; 18 Feb 1998 11:14:14 -0800 X400-Received: by /c=us/admd=telemail/prmd=nasa/; Relayed; 18 Feb 1998 11:14:14 -0800 X400-MTS-Identifier: [/c=us/admd=telemail/prmd=nasa/; 035AA34EB3306066-Proteus] Content-Identifier: 035AA34EB3306066 Content-Return: Allowed X400-Content-Type: P2-1988 ( 22 ) Conversion: Allowed Original-Encoded-Information-Types: IA5-Text Priority: normal Disclose-Recipients: Prohibited Alternate-Recipient: Allowed X400-Originator: Paula.M.Eshe@jpl.nasa.gov X400-Recipients: non-disclosure; Message-Id: <035AA34EB3306066*/c=us/admd=telemail/prmd=nasa/o=jpl/ou=ccmail/s=Eshe/g=Paula/i=M/@MHS> Date: 18 Feb 1998 11:14:14 -0800 From: Paula M Eshe To: len@nova.Stanford.EDU (IPM Return requested), hinson@nimbus.Stanford.EDU (IPM Return requested), joe@neptune.Stanford.EDU (IPM Return requested), rsimpson@magellan.stanford.edu (IPM Return requested), Sami W Asmar (IPM Return requested), Salvatore F Abbate (IPM Return requested), Jennifer L Caetta (IPM Return requested), Patricia Priest (IPM Return requested) Subject: Occultation #33 MIME-Version: 1.0 Content-Length: 477 Status: O Hello Everything went well at DSS 25 for occultation #33. Record time: 049/18:05:23 to 049/18:40:35 One-way time: 049/18:26:45 to 049/18:39:39 Expected Surface: 049/18:37:39 SPK: spk_i_980217_OD136_146_V1 SOE: p137a.01.soe Script: 98049.25.a136.scr Three attenuation changes, the last one at 18:30:23. We had some trouble getting the DSP to go to run. So we started recording earlier. The next occultation occurs at 2:44 AM PST Thursday at DSS 54. Paula