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 1998/051." END_OBJECT = TEXT END From Paula.M.Eshe@jpl.nasa.gov Thu Feb 19 23:02:56 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 XAA15804 for ; Thu, 19 Feb 1998 23:02:55 -0800 (PST) Received: from jpl-mhs.jpl.nasa.gov by eis-msg-012.jpl.nasa.gov (X.400 to RFC822 Gateway); Thu, 19 Feb 1998 23:02:28 -0800 X400-Received: by mta Proteus in /c=us/admd=telemail/prmd=nasa/; Relayed; 19 Feb 1998 23:02:22 -0800 X400-Received: by /c=us/admd=telemail/prmd=nasa/; Relayed; 19 Feb 1998 23:02:22 -0800 X400-MTS-Identifier: [/c=us/admd=telemail/prmd=nasa/; 02DD434ED2A7E00C-Proteus] Content-Identifier: 02DD434ED2A7E00C 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: <02DD434ED2A7E00C*/c=us/admd=telemail/prmd=nasa/o=jpl/ou=ccmail/s=Eshe/g=Paula/i=M/@MHS> Date: 19 Feb 1998 23:02:22 -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), Salvatore F Abbate (IPM Return requested), Patricia Priest (IPM Return requested) Subject: Occultation #35 MIME-Version: 1.0 Content-Length: 378 Status: RO Hello Everything went well at DSS 45 for occultation #35. Record time: 051/02:39:00 to 051/02:53:00 One-way time: 051/02:39:37 to 051/02:52:30 Expected Surface: 051/02:50:29 SPK: spk_i_980218_OD138_148_V1 SOE: p139b.01.soe Script: 98051.45.a138.scr SNT: 29.13 No attenuation changes. The next occultation occurs at 10:50 AM PST Friday at DSS 25. Paula ----------------------------------------------------------------- From Paula.M.Eshe@jpl.nasa.gov Fri Feb 20 11:31:59 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 LAA23121 for ; Fri, 20 Feb 1998 11:31:59 -0800 (PST) Received: from jpl-mhs.jpl.nasa.gov by eis-msg-012.jpl.nasa.gov (X.400 to RFC822 Gateway); Fri, 20 Feb 1998 11:29:08 -0800 X400-Received: by mta Proteus in /c=us/admd=telemail/prmd=nasa/; Relayed; 20 Feb 1998 11:29:06 -0800 X400-Received: by /c=us/admd=telemail/prmd=nasa/; Relayed; 20 Feb 1998 11:29:06 -0800 X400-MTS-Identifier: [/c=us/admd=telemail/prmd=nasa/; 05A1634EDD982078-Proteus] Content-Identifier: 05A1634EDD982078 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: <05A1634EDD982078*/c=us/admd=telemail/prmd=nasa/o=jpl/ou=ccmail/s=Eshe/g=Paula/i=M/@MHS> Date: 20 Feb 1998 11:29:06 -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 #36 MIME-Version: 1.0 Content-Length: 513 Status: RO Hello Everything went well at DSS 25 for occultation #36. Dick, I watched the SSI the whole time we were recording. I did not see any spurs, I do see lots of little dots now. Record time: 051/18:38:00 to 051/18:52:00 One-way time: 051/18:38:27 to 051/18:51:19 Expected Surface: 051/18:49:19 SPK: spk_i_980219_OD149_V1 SOE: p140a.01.soe Script: 98051.25.a139.scr SNT: 39.56 No attenuation changes. The next occultation occurs at 02:47 AM PST Saturday at DSS 65. Have a nice weekend Paula ------------------------------------------------------------------ From hinson@nimbus.Stanford.EDU Mon Feb 23 12:43:47 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 MAA24618 for ; Mon, 23 Feb 1998 12:43:46 -0800 (PST) Received: (from hinson@localhost) by nimbus.Stanford.EDU (8.8.4/8.8.3) id MAA00281; Mon, 23 Feb 1998 12:43:39 -0800 (PST) Date: Mon, 23 Feb 1998 12:43:39 -0800 (PST) From: Dave Hinson Message-Id: <199802232043.MAA00281@nimbus.Stanford.EDU> To: joe@neptune.Stanford.EDU, rsimpson@magellan.Stanford.EDU Subject: dss25 X-Sun-Charset: US-ASCII Content-Length: 159 Status: R The most recent data from dss25 (80511838) have much noisier frequency residuals than the previous pass at that station (80491830). Any ideas as to why? -------------------------------------------------------------------- To: hinson@nimbus.Stanford.EDU, joe@neptune.Stanford.EDU From: rsimpson@magellan Subject: Re: dss25 Cc: >The most recent data from dss25 (80511838) have much noisier >frequency residuals than the previous pass at that station >(80491830). Any ideas as to why? Nothing obvious here. These data also have ~200 Hz spurs, but they are less pronounced than the spurs a couple days earlier. Everything else at the quick-look level looks fine.