PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2007-07-29 NOTE = " E-mail and other messages concerning MGS Radio Science on or about 2000/112." END_OBJECT = TEXT END From trish@rodan.jpl.nasa.gov Mon Apr 17 17:48 PDT 2000 Received: from godzilla.jpl.nasa.gov (godzilla.jpl.nasa.gov [137.78.177.120]) by magellan.stanford.edu (8.9.3/8.9.3) with ESMTP id RAA09277 for ; Mon, 17 Apr 2000 17:48:57 -0700 (PDT) Received: from 137.78.177.117 (trish-mac.jpl.nasa.gov [137.78.177.117]) by godzilla.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id RAA11516; Mon, 17 Apr 2000 17:48:56 -0700 (PDT) Message-Id: <200004180048.RAA11516@godzilla.jpl.nasa.gov> Date: 17 Apr 00 17:51:12 -0700 From: Trish Priest Subject: DSP Conflicts To: David Hinson , Richard Simpson , Joe Twicken , Len Tyler X-Mailer: QuickMail Pro 1.5.4 (Mac) X-Priority: 3 Reply-To: Trish Priest MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset="US-Ascii" Content-Length: 781 Status: RO Hello, Cassini, Galileo, and MGS all seem to be in the same part of the sky. Cassini has an HGA antenna boresight calibration on DOY 109 and 111, so MGS will not have the DSS for the SPC 10 passes on those two days. Galileo has the DSP on DOY 112 at SPC 60. The MGS pass was fairly short. Also, Galileo's solar conjunction period extends between April 21 and May 21, 2000. One of the German investigators (Rainer) will be at JPL, and Galileo will be sharing the DSP with MGS for that period. The GLL measurements should not impact MGS occultations very much. With a few exceptions, GLL will use the DSP either immediately before or after the MGS passes. At SPC 40, we will be utilizing both DSPs. This will be a bit more operationally intensive than usual. -Trish -------------------------------------------------------------------------- From ppriest@airmail.fltops.jpl.nasa.gov Fri Apr 21 01:15 PDT 2000 Received: from thorn.fltops.jpl.nasa.gov (thorn.fltops.jpl.nasa.gov [137.228.90.10]) by magellan.stanford.edu (8.9.3/8.9.3) with SMTP id BAA05633; Fri, 21 Apr 2000 01:15:58 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id BAA16223; Fri, 21 Apr 2000 01:15:58 -0700 Received: from airmail.fltops.jpl.nasa.gov(137.228.96.12) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma016198; Fri, 21 Apr 00 01:15:17 -0700 Received: from mmrs.fltops.jpl.nasa.gov (mmrs.fltops.jpl.nasa.gov [137.228.136.10]) by airmail.fltops.jpl.nasa.gov (8.9.3+Sun/8.9.3) with ESMTP id BAA24755; Fri, 21 Apr 2000 01:15:15 -0700 (PDT) Received: (from ppriest@localhost) by mmrs.fltops.jpl.nasa.gov (8.8.8+Sun/8.8.8) id IAA13102; Fri, 21 Apr 2000 08:15:11 GMT Date: Fri, 21 Apr 2000 08:15:11 GMT From: Patricia Priest Message-Id: <200004210815.IAA13102@mmrs.fltops.jpl.nasa.gov> DSS: 45 Apparently-To: Apparently-To: Content-Type: text Content-Length: 271 Status: RO Orbit: 5007i SOE: mm032a.06.tsoe Begin Record: 112/04:04:00 End Record: 112/04:11:00 Last Attenuation Change: SNT: Elevation Angle: Orbit: 5008i SOE: mm032a.06.tsoe Begin Record: 112/06:01:00 End Record: 112/06:09:00 Last Attenuation Change: SNT: Elevation Angle: -------------------------------------------------------------------------- From joe@neptune.stanford.edu Thu Apr 27 17:34 PDT 2000 Received: from nova.Stanford.EDU (nova [171.64.90.123]) by magellan.stanford.edu (8.9.3/8.9.3) with ESMTP id RAA20114 for ; Thu, 27 Apr 2000 17:34:31 -0700 (PDT) Received: from neptune.Stanford.EDU (neptune.Stanford.EDU [171.64.90.149]) by nova.Stanford.EDU (8.9.3/8.9.3) with ESMTP id RAA28761; Thu, 27 Apr 2000 17:34:34 -0700 (PDT) Received: (from joe@localhost) by neptune.Stanford.EDU (8.9.3/8.9.3) id RAA22168; Thu, 27 Apr 2000 17:30:26 -0700 (PDT) Message-ID: X-Mailer: XFMail 1.2 [p0] on Solaris X-Priority: 3 (Normal) Content-Transfer-Encoding: 8bit MIME-Version: 1.0 In-Reply-To: <200004280021.RAA19210@magellan.stanford.edu> Date: Thu, 27 Apr 2000 17:30:26 -0700 (PDT) Sender: joe@neptune.stanford.edu From: Joe Twicken To: joe@nova.stanford.edu, rsimpson@nova.stanford.edu, hinson@nova.stanford.edu Subject: RE: ODR Notice: /users/z19/procODR/01190016 Content-Type: text/plain; charset=us-ascii Content-Length: 350 Status: RO (1) There was no HGA motion compensation for these recordings On 28-Apr-00 Joe Twicken 723-3597 wrote: > 01120404.ODR p 45XRXIR1R201 45XRXIC1XX01 45XR1IF1S101 45XR1IS1T101 > 45XR1IS1T201 45XR1IS1T301 45XR1IS1T401 45XR1IS1T501 > 01120601.ODR p 45XRXIR1R201 45XRXIC1XX01 45XR1IF1S101 45XR1IS1T101 > 45XR1IS1T201 45XR1IS1T301 45XR1IS1T401 45XR1IS1T501 -------------------------------------------------------------------------- From joe@neptune.stanford.edu Thu Oct 11 09:39 PDT 2001 Received: from neptune.Stanford.EDU (neptune [171.64.90.149]) by magellan.stanford.edu (8.9.3/8.9.3) with ESMTP id JAA14155 for ; Thu, 11 Oct 2001 09:39:56 -0700 (PDT) Received: (from joe@localhost) by neptune.Stanford.EDU (8.9.3/8.9.3) id JAA26416; Thu, 11 Oct 2001 09:36:53 -0700 (PDT) Message-ID: X-Mailer: XFMail 1.2 [p0] on Solaris X-Priority: 3 (Normal) Content-Transfer-Encoding: 8bit MIME-Version: 1.0 In-Reply-To: <200110111630.JAA13369@magellan.stanford.edu> Date: Thu, 11 Oct 2001 09:36:52 -0700 (PDT) Sender: joe@neptune.stanford.edu From: Joe Twicken To: joe@nova.stanford.edu, rsimpson@magellan.stanford.edu, hinson@nova.stanford.edu Subject: RE: ODR Notice: /users/z13/procODR/12841622 Content-Type: text/plain; charset=us-ascii Content-Length: 408 Status: RO (1) Reprocessed with Goddard (ql18) trajectory (2) There was no HGA motion compensation for the 01120404.ODR recording On 11-Oct-01 Joe Twicken 723-3597 wrote: > 01120404.ODR p 45XRXIR1R202 45XRXIC1XX02 45XR1IF1S102 45XR1IS1T102 > 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502 > 01120601.ODR p 45XRXIR1R202 45XRXIC1XX02 45XR1IF1S102 45XR1IS1T102 > 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502