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 1998/068." END_OBJECT = TEXT END From trish@rodan.jpl.nasa.gov Mon Mar 9 00:11:35 1998 Received: from rodan.Jpl.Nasa.Gov (rodan.jpl.nasa.gov [128.149.43.24]) by magellan.Stanford.EDU (8.8.5/8.8.3) with ESMTP id AAA22684 for ; Mon, 9 Mar 1998 00:11:34 -0800 (PST) Received: from 128.149.43.27 (trish-mac.jpl.nasa.gov [128.149.43.27]) by rodan.Jpl.Nasa.Gov (8.8.5/8.6.6) with SMTP id AAA04519; Mon, 9 Mar 1998 00:11:33 -0800 (PST) Message-Id: <199803090811.AAA04519@rodan.Jpl.Nasa.Gov> Date: 09 Mar 98 00:13:37 -0800 From: Trish Priest Subject: Occultation #63, Orbit 166 To: David Hinson , Richard Simpson , Joe Twicken , Len Tyler CC: Salvadore Abbate , Sami Asmar , Jennifer Caetta , Paula Eshe X-Mailer: QuickMail Pro 1.0.2d1 X-Priority: 3 Reply-To: Trish Priest Content-Type: text/plain; charset="iso-8859-1" Content-Length: 844 Status: R Hello, The buffer error problem occurred again at SPC 40. Dick reports that there were some missing records and almost every record was duplicated twice for occultation 61 data. This error does not appear until the DSP begins recording. After the occultation was complete, I had the station reboot the DSP, and I ran it again. It continued to produce buffer errors. I will talk to Sal tomorrow, and we will use the other DSP at SPC 40 until this is resolved. Record Times: 068-07:08:00 to 068-07:27:00 One-way Times: 068-07:08:50 to 068-07:26:37 Expected Surface Begin: 068-07:21:38 Expected Eclipse Begin: 068-07:23:32 SNT: 48.22 SPK: spk_i_980308_OD166_196_V1 SOE: p166a.01.soe Script: 98068.34.a166.scr The last attenuation change occurred at 07:09:47. The next occultation occurs at 1:00 PM PST Monday. -Trish ----------------------------------------------------------------------- From Paula.M.Eshe@jpl.nasa.gov Mon Mar 9 13:23:36 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 NAA02008 for ; Mon, 9 Mar 1998 13:23:36 -0800 (PST) Received: from jpl-mhs.jpl.nasa.gov by eis-msg-012.jpl.nasa.gov (X.400 to RFC822 Gateway); Mon, 9 Mar 1998 13:20:51 -0800 X400-Received: by mta Proteus in /c=us/admd=telemail/prmd=nasa/; Relayed; 09 Mar 1998 13:20:47 -0800 X400-Received: by /c=us/admd=telemail/prmd=nasa/; Relayed; 09 Mar 1998 13:20:47 -0800 X400-MTS-Identifier: [/c=us/admd=telemail/prmd=nasa/; 0057735045D2F018-Proteus] Content-Identifier: 0057735045D2F018 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: <0057735045D2F018*/c=us/admd=telemail/prmd=nasa/o=jpl/ou=ccmail/s=Eshe/g=Paula/i=M/@MHS> Date: 09 Mar 1998 13:20:47 -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), Salvatore F Abbate (IPM Return requested), Sami W Asmar (IPM Return requested), Jennifer L Caetta (IPM Return requested), Patricia Priest (IPM Return requested) Subject: Occultation # 64 MIME-Version: 1.0 Content-Length: 409 Status: R Hello Everything went well with Occultation #64 at DSS 15. Record times: 068/20:47:00 to 068/21:06:00 One-way times: 068/20:47:32 to 068/21:05:19 Expected Surface: 068/21:00:19 Expected Eclipse: 068/21:02:26 SNT: 29.08 SOE: p168a.01.soe SPK: spk_i_980308_OD167_177_V1 Script: 98068.15.a167.scr No attenuation changes. The next Occultation occurs at 2:34 AM PST Tuesday at DSS 54. Paula ------------------------------------------------------------------- From joe@nova.Stanford.EDU Tue Mar 10 10:18:49 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 KAA10171 for ; Tue, 10 Mar 1998 10:18:49 -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 KAA24612; Tue, 10 Mar 1998 10:18:47 -0800 (PST) Received: (from joe@localhost) by neptune.Stanford.EDU (8.8.5/8.8.3) id KAA09422; Tue, 10 Mar 1998 10:14:36 -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 In-Reply-To: <199803101811.KAA10037@magellan.Stanford.EDU> Date: Tue, 10 Mar 1998 10:14:35 -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 Subject: RE: ODR Notice: /users/z11/procODR/80691808 Content-Length: 290 Status: RO Note that there were two POCA errors of the 100 microHertz variety which were auto-fixed. The time tags were 75589 and 75859; the latter occurred very close to the occultation... On 10-Mar-98 Joe Twicken 723-3597 wrote: > 80682047.ODR p 15XRXIR1R201 15XRXIC1XX01 15XR1IF1S101 15XR1IS1T101 ----------------------------------------------------------------------- From rsimpson Tue Mar 10 14:50:59 1998 Received: (from rsimpson@localhost) by magellan.Stanford.EDU (8.8.5/8.8.3) id OAA13448; Tue, 10 Mar 1998 14:50:55 -0800 (PST) Date: Tue, 10 Mar 1998 14:50:55 -0800 (PST) From: Dick Simpson 723-3525 Message-Id: <199803102250.OAA13448@magellan.Stanford.EDU> To: Jennifer.L.Caetta@jpl.nasa.gov, Patricia.Priest@jpl.nasa.gov, Paula.M.Eshe@jpl.nasa.gov, Salvatore.F.Abbate@jpl.nasa.gov, Sami.W.Asmar@jpl.nasa.gov, hinson@nimbus.Stanford.EDU, joe@neptune.Stanford.EDU, len@nova.Stanford.EDU, rsimpson@magellan.Stanford.EDU Subject: Occ #63 Content-Length: 414 Status: RO Looks good. More than one duplicate for every legitimate record. But no missing records, and all the data for the time interval requested was delivered by the Query Server. The amplitude baseline doesn't appear to be as good in these data, but that's an analysis issue. It appears that we (Trish) managed to pull #63 out of the fire with the retransmission. #65 arrived in the same batch. It also looks good.