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 2000/272." END_OBJECT = TEXT END From sami.asmar@jpl.nasa.gov Wed Aug 9 13:17 PDT 2000 Received: from eis-msg-014.jpl.nasa.gov (eis-msg-014.jpl.nasa.gov [137.78.160.158]) by magellan.stanford.edu (8.9.3/8.9.3) with ESMTP id NAA25477 for ; Wed, 9 Aug 2000 13:17:16 -0700 (PDT) Received: from asmar-nt (asmar-nt.jpl.nasa.gov [137.78.177.111]) by eis-msg-014.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id NAA13208; Wed, 9 Aug 2000 13:16:24 -0700 (PDT) Message-Id: <3.0.5.32.20000809131622.00bcd450@pop.jpl.nasa.gov> X-Sender: asmar@pop.jpl.nasa.gov X-Mailer: QUALCOMM Windows Eudora Pro Version 3.0.5 (32) Date: Wed, 09 Aug 2000 13:16:22 -0700 To: "Peter W. Tay" , hinson@nimbus.stanford.edu, rsimpson@magellan.stanford.edu, thomas.thorpe@jpl.nasa.gov, len@nova.stanford.edu From: Sami Asmar Subject: Re: DSP-R conflicts (MGS/CAS) Cc: Belinda.Arroyo@jpl.nasa.gov, kyetter@mail1.jpl.nasa.gov, aseel@godzilla.jpl.nasa.gov, Trina.L.Ray@jpl.nasa.gov, blandry@mail1.jpl.nasa.gov In-Reply-To: <3.0.32.20000809112249.00bc6cb0@pop.jpl.nasa.gov> Mime-Version: 1.0 Content-Type: text/enriched; charset="us-ascii" Content-Length: 1362 Status: RO Peter, Yes, I am afraid we at MGS have to give the DSP for these important Cassini HGA calibration and USO activities for four passes. I am looking into if we can share the last pass on DOY 272 if they don't need it for the entire pass. I will inform the MGS investigators and Project of the limited loss of RS occultation data. Sami At 11:22 AM 8/9/2000 -0700, Peter W. Tay wrote: >>>> Sami, CAS requested the DSP-R usage for the following passes, and they are in partial conflicts with the exception of Doy 272, which is a direct overlap with MGS. Are we relinquishing the MGS DSP-R to CAS? Please advise. Week 38 ---------- 267 0810 0910 1710 1725 DSS-25 CAS TP RSS QUIET TST V0071A1 267 1115 1215 2345 0000 DSS-15 MGS TKG PASS V4021A1 Week 39 --------- 269 0510 0610 1445 1500 DSS-25 CAS TP RSSUSO/HGACAL V0071A1 269 1115 1215 2000 2015 DSS-15 MGS TKG PASS V4021A1 271 0515 0615 1835 1850 DSS-25 CAS TP RSS HGA P/CAL V0071A1 271 1445 1545 2110 2125 DSS-15 MGS TKG PASS V4021A1 272 0500 0600 1835 1850 DSS-25 CAS TP RWAFRT/RS T-D V0071A1 272 1115 1215 1645 1700 DSS-15 MGS TKG PASS V4021A1 Peter -------------------------------------------------------------------------- From sami.asmar@jpl.nasa.gov Wed Aug 9 16:05 PDT 2000 Received: from eis-msg-014.jpl.nasa.gov (eis-msg-014.jpl.nasa.gov [137.78.160.158]) by magellan.stanford.edu (8.9.3/8.9.3) with ESMTP id QAA08914 for ; Wed, 9 Aug 2000 16:05:19 -0700 (PDT) Received: from asmar-nt (asmar-nt.jpl.nasa.gov [137.78.177.111]) by eis-msg-014.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id QAA07759; Wed, 9 Aug 2000 16:05:18 -0700 (PDT) Message-Id: <3.0.5.32.20000809160516.00b54100@pop.jpl.nasa.gov> X-Sender: asmar@pop.jpl.nasa.gov X-Mailer: QUALCOMM Windows Eudora Pro Version 3.0.5 (32) Date: Wed, 09 Aug 2000 16:05:16 -0700 To: Dave Hinson From: Sami Asmar Subject: Cassini DSP needs in September Cc: len@nova.stanford.edu, rsimpson@magellan.stanford.edu In-Reply-To: <200008092121.OAA12495@nimbus.Stanford.EDU> Mime-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Length: 2483 Status: O Sami, Half of the Cassini activities in late September 2000 are Instrument Check-Out (ICO) #2 activities. The first ICO occurred in January 1999 and consisted of 8 tracks of observations. ICO #1 was our first opportunity to test the functionality of the the Cassini RS System. As a reminder, Cassini is the first spacecraft with specific Radio Science hardware on-board (not including USOs). On DOY 267, we will be repeating the RSS Quiet Test. The RSS Quiet Test was a test designed to allow Radio Science to "listen" to the other instruments so that we could determine how "noisy" they are. After analyzing the data from ICO #1, we determined that this test failed. On DOY 272, we will be doing Test D, an X-up/Ka-down test. Since we were on thrusters and not reaction wheels during ICO #1, we knew that we'd have to re-do this test. The other half of our activities are normal calibrations. On DOY 269, we will be doing a USO Test and a boresight calibration. The X-band and Ka-band boresights are slightly offset. We also expect them to drift slightly over time. One of the requirements for the GWE is that we update the Ka-band boresight within 30 days of the start of the experiment. We need time to validate and verify that process. On DOY 271, we will be doing pattern calibrations for both the X-band and Ka-band. These cannot be done simultaneously because each frequency band requires different endpoints and slew rates. Each of these calibrations takes about 4.5 hours. These activities were grouped together because of a concern from the Huygens Probe regarding our S-band Transmitter (SBT). The Probe observes a large thermal cycle everytime we turn ON the SBT. By keeping our calibrations close together, we can limit the thermal cycles to one. (The RST and the Probe have agreed that we would limit such cycles to less than 50 before the end of Probe mission. We have had about 10 cycles so far.) Best, Randy At 02:21 PM 8/9/2000 -0700, Dave Hinson wrote: >Sami, > >I'm happy to accommodate the Cassini requests provided >that they are reasonable. But it's not obvious to me >why four passes are needed for "HGA calibration and USO >activities." USO tests during MGS cruise lasted only >about 1-2 hours, but maybe there's a good reason for the >difference. > >Your first message also made it sound as though the matter >was settled, which prompted my question about how these >conflicts are resolved. > >Regards, >Dave -------------------------------------------------------------------------- From ppriest@airmail.fltops.jpl.nasa.gov Wed Sep 27 22:29 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 WAA16596; Wed, 27 Sep 2000 22:29:34 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id WAA05370; Wed, 27 Sep 2000 22:30:21 -0700 Received: from airmail.fltops.jpl.nasa.gov(137.228.96.12) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma005355; Wed, 27 Sep 00 22:30:11 -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 WAA27235; Wed, 27 Sep 2000 22:30:10 -0700 (PDT) Received: (from ppriest@localhost) by mmrs.fltops.jpl.nasa.gov (8.8.8+Sun/8.8.8) id FAA21111; Thu, 28 Sep 2000 05:30:10 GMT Date: Thu, 28 Sep 2000 05:30:10 GMT From: Patricia Priest Message-Id: <200009280530.FAA21111@mmrs.fltops.jpl.nasa.gov> DSS: 34 Apparently-To: Apparently-To: Content-Type: text Content-Length: 138 Status: RO Orbit: 6965i SOE: mm074b.01.tsoe Begin Record: 272/03:41:00 End Record: 272/03:48:00 Last Attenuation Change: SNT: Elevation Angle: -------------------------------------------------------------------------- From ppriest@airmail.fltops.jpl.nasa.gov Thu Sep 28 06:14 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 GAA16958; Thu, 28 Sep 2000 06:14:40 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id GAA08015; Thu, 28 Sep 2000 06:15:27 -0700 Received: from airmail.fltops.jpl.nasa.gov(137.228.96.12) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma007769; Thu, 28 Sep 00 06:15:12 -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 GAA03112; Thu, 28 Sep 2000 06:15:11 -0700 (PDT) Received: (from ppriest@localhost) by mmrs.fltops.jpl.nasa.gov (8.8.8+Sun/8.8.8) id NAA21242; Thu, 28 Sep 2000 13:15:11 GMT Date: Thu, 28 Sep 2000 13:15:11 GMT From: Patricia Priest Message-Id: <200009281315.NAA21242@mmrs.fltops.jpl.nasa.gov> DSS: 54 Apparently-To: Apparently-To: Content-Type: text Content-Length: 538 Status: RO Orbit: 6966i SOE: mm074b.01.tsoe Begin Record: 272/05:39:00 End Record: 272/05:46:00 Last Attenuation Change: SNT: Elevation Angle: Orbit: 6967i SOE: mm074b.01.tsoe Begin Record: 272/07:37:00 End Record: 272/07:44:00 Last Attenuation Change: SNT: Elevation Angle: Orbit: 6968i SOE: mm074b.01.tsoe Begin Record: 272/09:34:00 End Record: 272/09:41:00 Last Attenuation Change: SNT: Elevation Angle: Orbit: 6969i SOE: mm074b.01.tsoe Begin Record: 272/11:32:00 End Record: 272/11:39:00 Last Attenuation Change: SNT: Elevation Angle: -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Thu Sep 28 06:02 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 GAA16924 for ; Thu, 28 Sep 2000 06:02:44 -0700 (PDT) Received: from localhost (localhost [127.0.0.1]) by godzilla.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id GAA15225 for ; Thu, 28 Sep 2000 06:03:31 -0700 (PDT) Message-Id: <200009281303.GAA15225@godzilla.jpl.nasa.gov> Date: Thu, 28 Sep 2000 06:03:31 -0700 (PDT) From: Aseel Anabtawi Reply-To: Aseel Anabtawi Subject: 2000/272 at DSS 15 To: rsimpson@magellan.stanford.edu MIME-Version: 1.0 Content-MD5: Nn9uiUIvElRhPhCXsx2H9Q== X-Mailer: dtmail 1.2.1 CDE Version 1.2.1 SunOS 5.6 sun4u sparc Content-Type: TEXT/plain; charset=us-ascii Content-Length: 62 Status: RO Cassini has the DSP, so no data is collected over this pass. -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Thu Sep 28 05:58 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 FAA16894 for ; Thu, 28 Sep 2000 05:58:33 -0700 (PDT) Received: from localhost (localhost [127.0.0.1]) by godzilla.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id FAA15211 for ; Thu, 28 Sep 2000 05:59:20 -0700 (PDT) Message-Id: <200009281259.FAA15211@godzilla.jpl.nasa.gov> Date: Thu, 28 Sep 2000 05:59:20 -0700 (PDT) From: Aseel Anabtawi Reply-To: Aseel Anabtawi Subject: 2000/271 at DSS 34 To: rsimpson@magellan.stanford.edu MIME-Version: 1.0 Content-MD5: P2fVHlTaNmoU7azY0aDRaQ== X-Mailer: dtmail 1.2.1 CDE Version 1.2.1 SunOS 5.6 sun4u sparc Content-Type: TEXT/plain; charset=us-ascii Content-Length: 172 Status: O Hello, I had to monitor this one from home. The script ran OK, but the RMS values were low, so either the attenuation values were off, or there was no signal. -Aseel -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Thu Sep 28 06:02 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 GAA16914 for ; Thu, 28 Sep 2000 06:02:29 -0700 (PDT) Received: from localhost (localhost [127.0.0.1]) by godzilla.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id GAA15221 for ; Thu, 28 Sep 2000 06:03:16 -0700 (PDT) Message-Id: <200009281303.GAA15221@godzilla.jpl.nasa.gov> Date: Thu, 28 Sep 2000 06:03:16 -0700 (PDT) From: Aseel Anabtawi Reply-To: Aseel Anabtawi Subject: 272 not 271 at DSS 34 To: rsimpson@magellan.stanford.edu MIME-Version: 1.0 Content-MD5: 2AQA5iv5zwsyNCiM8i+UPA== X-Mailer: dtmail 1.2.1 CDE Version 1.2.1 SunOS 5.6 sun4u sparc Content-Type: TEXT/plain; charset=us-ascii Content-Length: 85 Status: RO Sorry, I meant 272 in the subject. There was only one measurement over this pass. -------------------------------------------------------------------------- From ppriest@airmail.fltops.jpl.nasa.gov Thu Sep 28 22:25 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 WAA13864; Thu, 28 Sep 2000 22:25:20 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id WAA20522; Thu, 28 Sep 2000 22:26:08 -0700 Received: from airmail.fltops.jpl.nasa.gov(137.228.96.12) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma019754; Thu, 28 Sep 00 22:25:12 -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 WAA17431; Thu, 28 Sep 2000 22:25:10 -0700 (PDT) Received: (from ppriest@localhost) by mmrs.fltops.jpl.nasa.gov (8.8.8+Sun/8.8.8) id FAA21899; Fri, 29 Sep 2000 05:25:11 GMT Date: Fri, 29 Sep 2000 05:25:11 GMT From: Patricia Priest Message-Id: <200009290525.FAA21899@mmrs.fltops.jpl.nasa.gov> DSS: 45 Apparently-To: Apparently-To: Content-Type: text Content-Length: 537 Status: R Orbit: 6974i SOE: mm074b.01.tsoe Begin Record: 272/21:20:00 End Record: 272/21:27:00 Last Attenuation Change: SNT: Elevation Angle: Orbit: 6975i SOE: mm074b.01.tsoe Begin Record: 272/23:18:00 End Record: 272/23:25:00 Last Attenuation Change: SNT: Elevation Angle: Orbit: 6976i SOE: mm074b.01.tsoe Begin Record: 273/01:16:00 End Record: 273/01:23:00 Last Attenuation Change: SNT: Elevation Angle: Orbit: 6977i SOE: mm074b.01.tsoe Begin Record: 273/03:13:00 End Record: 273/03:20:00 Last Attenuation Change: SNT: Elevation Angle: -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Fri Sep 29 02:13 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 CAA14004 for ; Fri, 29 Sep 2000 02:13:52 -0700 (PDT) Received: from localhost (localhost [127.0.0.1]) by godzilla.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id CAA19456 for ; Fri, 29 Sep 2000 02:14:40 -0700 (PDT) Message-Id: <200009290914.CAA19456@godzilla.jpl.nasa.gov> Date: Fri, 29 Sep 2000 02:14:40 -0700 (PDT) From: Aseel Anabtawi Reply-To: Aseel Anabtawi Subject: 2000/272 at DSS 45 To: rsimpson@magellan.stanford.edu MIME-Version: 1.0 Content-MD5: GCXI3XoRLNOI4Wav8BTy6g== X-Mailer: dtmail 1.2.1 CDE Version 1.2.1 SunOS 5.6 sun4u sparc Content-Type: TEXT/plain; charset=us-ascii Content-Length: 125 Status: R Hello, DSN predicts were used for the first measurement (6974i). Our predicts were used for the remaining three. -Aseel -------------------------------------------------------------------------- From joe@neptune.stanford.edu Thu Oct 19 15:11 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 PAA19640 for ; Thu, 19 Oct 2000 15:11:32 -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 PAA11814; Thu, 19 Oct 2000 15:12:46 -0700 (PDT) Received: (from joe@localhost) by neptune.Stanford.EDU (8.9.3/8.9.3) id PAA12891; Thu, 19 Oct 2000 15:11:52 -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: <200010192152.OAA16693@magellan.stanford.edu> Date: Thu, 19 Oct 2000 15:11:51 -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/02932139 Content-Type: text/plain; charset=us-ascii Content-Length: 1135 Status: RO (1) The following recordings were possibly contaminated by momentum desaturations: 02720934.ODR: desaturation from 2000/272-09:07:06.000 to 2000/272-09:10:18.000 Note that the one-way light time was approximately 20:33 on the date of the recording (2) There was no HGA motion compensation for these recordings On 19-Oct-00 Joe Twicken 723-3597 wrote: > 02720539.ODR p 54XRXIR1R201 54XRXIC1XX01 54XR1IF1S101 54XR1IS1T101 > 54XR1IS1T201 54XR1IS1T301 54XR1IS1T401 54XR1IS1T501 > 02720737.ODR p 54XRXIR1R201 54XRXIC1XX01 54XR1IF1S101 54XR1IS1T101 > 54XR1IS1T201 54XR1IS1T301 54XR1IS1T401 54XR1IS1T501 > 02720934.ODR p 54XRXIR1R201 54XRXIC1XX01 54XR1IF1S101 54XR1IS1T101 > 54XR1IS1T201 54XR1IS1T301 54XR1IS1T401 54XR1IS1T501 > 02721132.ODR p 54XRXIR1R201 54XRXIC1XX01 54XR1IF1S101 54XR1IS1T101 > 54XR1IS1T201 54XR1IS1T301 54XR1IS1T401 54XR1IS1T501 > 02722120.ODR p 45XRXIR1R201 45XRXIC1XX01 45XR1IF1S101 45XR1IS1T101 > 45XR1IS1T201 45XR1IS1T301 45XR1IS1T401 45XR1IS1T501 > 02722318.ODR p 45XRXIR1R201 45XRXIC1XX01 45XR1IF1S101 45XR1IS1T101 > 45XR1IS1T201 45XR1IS1T301 45XR1IS1T401 45XR1IS1T501 -------------------------------------------------------------------------- From joe@neptune.stanford.edu Mon Jul 30 14:53 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 OAA26976 for ; Mon, 30 Jul 2001 14:53:26 -0700 (PDT) Received: (from joe@localhost) by neptune.Stanford.EDU (8.9.3/8.9.3) id OAA14796; Mon, 30 Jul 2001 14:51:39 -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: <200107302142.OAA26923@magellan.stanford.edu> Date: Mon, 30 Jul 2001 14:51:39 -0700 (PDT) Sender: joe@neptune.stanford.edu From: Joe Twicken To: rsimpson@magellan.stanford.edu, hinson@nova.stanford.edu Subject: RE: ODR Notice: /users/z15/procODR/12112129 Content-Type: text/plain; charset=us-ascii Content-Length: 476 Status: RO Please disregard this one too. The correct one is coming. Sorry. On 30-Jul-01 Joe Twicken 723-3597 wrote: > 02721132.ODR p 54XRXIR1R202 54XRXIC1XX02 54XR1IF1S102 54XR1IS1T102 > 54XR1IS1T202 54XR1IS1T302 54XR1IS1T402 54XR1IS1T502 > 02722120.ODR p 45XRXIR1R202 45XRXIC1XX02 45XR1IF1S102 45XR1IS1T102 > 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502 > 02722318.ODR p 45XRXIR1R202 45XRXIC1XX02 45XR1IF1S102 45XR1IS1T102 > 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502 -------------------------------------------------------------------------- From joe@neptune.stanford.edu Mon Jul 30 15:04 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 PAA27032 for ; Mon, 30 Jul 2001 15:04:02 -0700 (PDT) Received: (from joe@localhost) by neptune.Stanford.EDU (8.9.3/8.9.3) id PAA14813; Mon, 30 Jul 2001 15:02:15 -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: <200107302155.OAA26987@magellan.stanford.edu> Date: Mon, 30 Jul 2001 15:02:15 -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/z15/procODR/12112129 Content-Type: text/plain; charset=us-ascii Content-Length: 1236 Status: RO (1) Reprocessed with Goddard trajectory. I am sorry about the myriad of problems I had with this one. I made it much more complicated than it needed to be (2) The following recordings were possibly contaminated by momentum desaturations: 02720934.ODR: desaturation from 2000/272-09:07:06.000 to 2000/272-09:10:18.000 Note that the one-way light time was approximately 20:33 on the date of the recording On 30-Jul-01 Joe Twicken 723-3597 wrote: > 02720539.ODR p 54XRXIR1R202 54XRXIC1XX02 54XR1IF1S102 54XR1IS1T102 > 54XR1IS1T202 54XR1IS1T302 54XR1IS1T402 54XR1IS1T502 > 02720737.ODR p 54XRXIR1R202 54XRXIC1XX02 54XR1IF1S102 54XR1IS1T102 > 54XR1IS1T202 54XR1IS1T302 54XR1IS1T402 54XR1IS1T502 > 02720934.ODR p 54XRXIR1R202 54XRXIC1XX02 54XR1IF1S102 54XR1IS1T102 > 54XR1IS1T202 54XR1IS1T302 54XR1IS1T402 54XR1IS1T502 > 02721132.ODR p 54XRXIR1R202 54XRXIC1XX02 54XR1IF1S102 54XR1IS1T102 > 54XR1IS1T202 54XR1IS1T302 54XR1IS1T402 54XR1IS1T502 > 02722120.ODR p 45XRXIR1R202 45XRXIC1XX02 45XR1IF1S102 45XR1IS1T102 > 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502 > 02722318.ODR p 45XRXIR1R202 45XRXIC1XX02 45XR1IF1S102 45XR1IS1T102 > 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502