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 1998/063." END_OBJECT = TEXT END From Paula.M.Eshe@jpl.nasa.gov Tue Mar 3 18:00:03 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 SAA12492 for ; Tue, 3 Mar 1998 18:00:02 -0800 (PST) Received: from jpl-mhs.jpl.nasa.gov by eis-msg-012.jpl.nasa.gov (X.400 to RFC822 Gateway); Tue, 3 Mar 1998 18:00:00 -0800 X400-Received: by mta Proteus in /c=us/admd=telemail/prmd=nasa/; Relayed; 03 Mar 1998 17:59:59 -0800 X400-Received: by /c=us/admd=telemail/prmd=nasa/; Relayed; 03 Mar 1998 17:59:59 -0800 X400-MTS-Identifier: [/c=us/admd=telemail/prmd=nasa/; 017D334FCB59F107-Proteus] Content-Identifier: 017D334FCB59F107 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: <017D334FCB59F107*/c=us/admd=telemail/prmd=nasa/o=jpl/ou=ccmail/s=Eshe/g=Paula/i=M/@MHS> Date: 03 Mar 1998 17:59:59 -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 # 54 MIME-Version: 1.0 Content-Length: 491 Status: RO Hello Everything went well for Occultation #54 at DSS15. Record times: 063/01:38:00 to 01:57:00 One-way times: 063/01:38:48 to 01:56:36 Expected Surface: 063/01:51:36 SNT: 34.95 SOE: p158.01.soe SPK: spk_i_980302_OD157_167_V1 Script: 98063.15.a157.scr One attenuation cahange at 01:40:00. The next occultation occurs at 8:08 AM PST Wednesday at DSS 65. Paula ---------------------------------------------------------------- From Paula.M.Eshe@jpl.nasa.gov Wed Mar 4 08:21:29 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 IAA18528 for ; Wed, 4 Mar 1998 08:21:29 -0800 (PST) Received: from jpl-mhs.jpl.nasa.gov by eis-msg-012.jpl.nasa.gov (X.400 to RFC822 Gateway); Wed, 4 Mar 1998 08:21:26 -0800 X400-Received: by mta Proteus in /c=us/admd=telemail/prmd=nasa/; Relayed; 04 Mar 1998 08:21:24 -0800 X400-Received: by /c=us/admd=telemail/prmd=nasa/; Relayed; 04 Mar 1998 08:21:24 -0800 X400-MTS-Identifier: [/c=us/admd=telemail/prmd=nasa/; 04E9F34FD7F840C3-Proteus] Content-Identifier: 04E9F34FD7F840C3 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: <04E9F34FD7F840C3*/c=us/admd=telemail/prmd=nasa/o=jpl/ou=ccmail/s=Eshe/g=Paula/i=M/@MHS> Date: 04 Mar 1998 08:21:24 -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 #55 MIME-Version: 1.0 Content-Length: 369 Status: R Hello Everything went well for Occultation #55 at DSS 65. Record times: 063/15:55:00 to 063/16:14:00 One-way times: 063/15:55:41 to 063/16:13:28 Expected Surface: 063/16:08:29 SNT: 30.16 SOE: p158a.01.soe SPK: spk_i_980303_OD158_168_V1 SCRIPT: 98063.65.a158.scr No attenuation changes. The next occultation occurs at 10:19 PM at DSS 34. Paula --------------------------------------------------------------------- From joe@nova.Stanford.EDU Thu Mar 5 11:30:00 1998 Received: from nova.stanford.edu (nova.Stanford.EDU [36.10.0.123]) by magellan.Stanford.EDU (8.8.5/8.8.3) with ESMTP id LAA07428 for ; Thu, 5 Mar 1998 11:30:00 -0800 (PST) Received: from neptune.Stanford.EDU (neptune.Stanford.EDU [36.10.0.149]) by nova.stanford.edu (8.8.8/8.8.4) with ESMTP id LAA01268; Thu, 5 Mar 1998 11:29:55 -0800 (PST) Received: (from joe@localhost) by neptune.Stanford.EDU (8.8.5/8.8.3) id LAA06025; Thu, 5 Mar 1998 11:25:49 -0800 (PST) Message-ID: X-Mailer: XFMail 1.2 [p0] on Solaris X-Priority: 3 (Normal) Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 8bit MIME-Version: 1.0 Date: Thu, 05 Mar 1998 11:25:48 -0800 (PST) Sender: joe@neptune.Stanford.EDU From: Joe Twicken To: stoumpis@leland.stanford.edu, joe@nova.Stanford.EDU, rsimpson@nova.Stanford.EDU, hinson@nova.Stanford.EDU, len@nova.Stanford.EDU, trish@zygra.jpl.nasa.gov Subject: USO Allan Deviation: Occultation #54 Content-Length: 570 Status: RO Hello all- I have estimated the USO Allan Deviation for the (approximately) 10 minute period of the occultation #54 recording prior to the beginning of the atmospheric occultation. The data were recorded at DSS 15 on 1998/063. t (sec) AD ------- ---------- 0.4096 1.4646e-12 1.6384 5.1309e-13 3.7268 3.7488e-13 6.5536 3.0399e-13 26.2144 3.4541e-13 Note that there are not very many samples from which to estimate Allan Deviation at the longest integration time. Joe