PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2007-07-31 NOTE = " E-mail and other messages concerning MGS Radio Science on or about 2002/134." END_OBJECT = TEXT END From aseel@airmail.fltops.jpl.nasa.gov Tue May 14 05:05:29 2002 Received: from thorn.fltops.jpl.nasa.gov (thorn.fltops.jpl.nasa.gov [137.228.90.10]) by magellan.stanford.edu (8.11.6/8.11.6) with SMTP id g4E44bJ12570; Mon, 13 May 2002 21:04:37 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id VAA14599; Mon, 13 May 2002 21:05:24 -0700 Received: from airmail1.fltops.jpl.nasa.gov(137.228.96.26) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma014508; Mon, 13 May 02 21:05:02 -0700 Received: from rsops2.fltops.jpl.nasa.gov (rsops2.fltops.jpl.nasa.gov [137.228.136.22]) by airmail1.fltops.jpl.nasa.gov (Postfix) with ESMTP id 19AA015BA; Tue, 14 May 2002 04:47:50 -0700 (PDT) Received: (from aseel@localhost) by rsops2.fltops.jpl.nasa.gov (8.10.2+Sun/8.10.2) id g4E452T09716; Tue, 14 May 2002 04:05:02 GMT Date: Tue, 14 May 2002 04:05:02 GMT From: aseel anabtawi Message-Id: <200205140405.g4E452T09716@rsops2.fltops.jpl.nasa.gov> To: aseel.anabtawi@jpl.nasa.gov, data@magellan.stanford.edu, joe@neptune.stanford.edu, kusza@magellan.stanford.edu, rsimpson@magellan.stanford.edu Content-Length: 1149 DSS: 25 RSR: RSR2A Subchannel: 1 Orbit Number: 14214 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/133-19:59:00 End Record: 2002/133-20:10:00 DSS: 25 RSR: RSR2A Subchannel: 1 Orbit Number: 14215 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/133-21:57:00 End Record: 2002/133-22:08:00 DSS: 25 RSR: RSR2A Subchannel: 1 Orbit Number: 14216 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/133-23:55:00 End Record: 2002/134-00:05:00 DSS: 25 RSR: RSR2A Subchannel: 1 Orbit Number: 14217 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-01:52:00 End Record: 2002/134-02:03:00 DSS: 25 RSR: RSR2A Subchannel: 1 Orbit Number: 14218 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-03:50:00 End Record: 2002/134-04:01:00 -------------------------------------------------------------------------- From aseel@airmail.fltops.jpl.nasa.gov Tue May 14 17:13:31 2002 Received: from thorn.fltops.jpl.nasa.gov (thorn.fltops.jpl.nasa.gov [137.228.90.10]) by magellan.stanford.edu (8.11.6/8.11.6) with SMTP id g4E7nSJ12922; Tue, 14 May 2002 00:49:28 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id AAA24776; Tue, 14 May 2002 00:50:14 -0700 Received: from airmail1.fltops.jpl.nasa.gov(137.228.96.26) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma024745; Tue, 14 May 02 00:50:02 -0700 Received: from rsops2.fltops.jpl.nasa.gov (rsops2.fltops.jpl.nasa.gov [137.228.136.22]) by airmail1.fltops.jpl.nasa.gov (Postfix) with ESMTP id B627915BA; Tue, 14 May 2002 08:32:49 -0700 (PDT) Received: (from aseel@localhost) by rsops2.fltops.jpl.nasa.gov (8.10.2+Sun/8.10.2) id g4E7o1609851; Tue, 14 May 2002 07:50:01 GMT Date: Tue, 14 May 2002 07:50:01 GMT From: aseel anabtawi Message-Id: <200205140750.g4E7o1609851@rsops2.fltops.jpl.nasa.gov> To: aseel.anabtawi@jpl.nasa.gov, data@magellan.stanford.edu, joe@neptune.stanford.edu, kusza@magellan.stanford.edu, rsimpson@magellan.stanford.edu Content-Length: 689 DSS: 45 RSR: RSR2A Subchannel: 1 Orbit Number: 14218 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-03:50:00 End Record: 2002/134-04:01:00 DSS: 45 RSR: RSR2A Subchannel: 1 Orbit Number: 14219 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-05:48:00 End Record: 2002/134-05:58:00 DSS: 45 RSR: RSR2A Subchannel: 1 Orbit Number: 14220 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-07:46:00 End Record: 2002/134-07:56:00 -------------------------------------------------------------------------- From aseel@airmail.fltops.jpl.nasa.gov Tue May 14 17:13:45 2002 Received: from thorn.fltops.jpl.nasa.gov (thorn.fltops.jpl.nasa.gov [137.228.90.10]) by magellan.stanford.edu (8.11.6/8.11.6) with SMTP id g4EDxvJ13154; Tue, 14 May 2002 06:59:57 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id HAA06524; Tue, 14 May 2002 07:00:44 -0700 Received: from airmail1.fltops.jpl.nasa.gov(137.228.96.26) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma006318; Tue, 14 May 02 07:00:02 -0700 Received: from rsops2.fltops.jpl.nasa.gov (rsops2.fltops.jpl.nasa.gov [137.228.136.22]) by airmail1.fltops.jpl.nasa.gov (Postfix) with ESMTP id 760FA15CE; Tue, 14 May 2002 14:42:50 -0700 (PDT) Received: (from aseel@localhost) by rsops2.fltops.jpl.nasa.gov (8.10.2+Sun/8.10.2) id g4EE01p10045; Tue, 14 May 2002 14:00:01 GMT Date: Tue, 14 May 2002 14:00:01 GMT From: aseel anabtawi Message-Id: <200205141400.g4EE01p10045@rsops2.fltops.jpl.nasa.gov> To: aseel.anabtawi@jpl.nasa.gov, data@magellan.stanford.edu, joe@neptune.stanford.edu, kusza@magellan.stanford.edu, rsimpson@magellan.stanford.edu Content-Length: 230 DSS: 54 RSR: RSR2A Subchannel: 1 Orbit Number: 14223 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-13:39:00 End Record: 2002/134-13:49:00 -------------------------------------------------------------------------- From aseel@airmail.fltops.jpl.nasa.gov Wed May 15 09:38:01 2002 Received: from thorn.fltops.jpl.nasa.gov (thorn.fltops.jpl.nasa.gov [137.228.90.10]) by magellan.stanford.edu (8.11.6/8.11.6) with SMTP id g4EKdpJ21570; Tue, 14 May 2002 13:39:51 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id NAA17904; Tue, 14 May 2002 13:40:39 -0700 Received: from airmail1.fltops.jpl.nasa.gov(137.228.96.26) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma017742; Tue, 14 May 02 13:40:01 -0700 Received: from rsops2.fltops.jpl.nasa.gov (rsops2.fltops.jpl.nasa.gov [137.228.136.22]) by airmail1.fltops.jpl.nasa.gov (Postfix) with ESMTP id 9E86A15D6; Tue, 14 May 2002 21:22:49 -0700 (PDT) Received: (from aseel@localhost) by rsops2.fltops.jpl.nasa.gov (8.10.2+Sun/8.10.2) id g4EKe1h10399; Tue, 14 May 2002 20:40:01 GMT Date: Tue, 14 May 2002 20:40:01 GMT From: aseel anabtawi Message-Id: <200205142040.g4EKe1h10399@rsops2.fltops.jpl.nasa.gov> To: aseel.anabtawi@jpl.nasa.gov, data@magellan.stanford.edu, joe@neptune.stanford.edu, kusza@magellan.stanford.edu, rsimpson@magellan.stanford.edu Content-Length: 919 DSS: 65 RSR: RSR2B Subchannel: 1 Orbit Number: 14223 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-13:39:00 End Record: 2002/134-13:49:00 DSS: 65 RSR: RSR2B Subchannel: 1 Orbit Number: 14224 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-15:36:00 End Record: 2002/134-15:47:00 DSS: 65 RSR: RSR2B Subchannel: 1 Orbit Number: 14225 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-17:34:00 End Record: 2002/134-17:45:00 DSS: 65 RSR: RSR2B Subchannel: 1 Orbit Number: 14226 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-19:32:00 End Record: 2002/134-19:43:00 -------------------------------------------------------------------------- From aseel@airmail.fltops.jpl.nasa.gov Wed May 15 09:32:02 2002 Received: from thorn.fltops.jpl.nasa.gov (thorn.fltops.jpl.nasa.gov [137.228.90.10]) by magellan.stanford.edu (8.11.6/8.11.6) with SMTP id g4F3j3J25485; Tue, 14 May 2002 20:45:03 -0700 (PDT) Received: by thorn.fltops.jpl.nasa.gov; id UAA19561; Tue, 14 May 2002 20:45:51 -0700 Received: from airmail1.fltops.jpl.nasa.gov(137.228.96.26) by thorn.fltops.jpl.nasa.gov via smap (V4.2) id xma019350; Tue, 14 May 02 20:45:02 -0700 Received: from rsops2.fltops.jpl.nasa.gov (rsops2.fltops.jpl.nasa.gov [137.228.136.22]) by airmail1.fltops.jpl.nasa.gov (Postfix) with ESMTP id 3121D15D9; Wed, 15 May 2002 04:27:49 -0700 (PDT) Received: (from aseel@localhost) by rsops2.fltops.jpl.nasa.gov (8.10.2+Sun/8.10.2) id g4F3j1O10882; Wed, 15 May 2002 03:45:01 GMT Date: Wed, 15 May 2002 03:45:01 GMT From: aseel anabtawi Message-Id: <200205150345.g4F3j1O10882@rsops2.fltops.jpl.nasa.gov> To: aseel.anabtawi@jpl.nasa.gov, data@magellan.stanford.edu, joe@neptune.stanford.edu, kusza@magellan.stanford.edu, rsimpson@magellan.stanford.edu Content-Length: 919 DSS: 24 RSR: RSR2A Subchannel: 1 Orbit Number: 14227 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-21:30:00 End Record: 2002/134-21:40:00 DSS: 24 RSR: RSR2A Subchannel: 1 Orbit Number: 14228 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/134-23:27:00 End Record: 2002/134-23:38:00 DSS: 24 RSR: RSR2A Subchannel: 1 Orbit Number: 14229 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/135-01:25:00 End Record: 2002/135-01:36:00 DSS: 24 RSR: RSR2A Subchannel: 1 Orbit Number: 14230 Occultation Sense: i SOE: mm177a.07.tsoe Ground Mode: 1 Uplink Station: -- Sampling Rate: 2K Bit Resolution: 16 Begin Record: 2002/135-03:23:00 End Record: 2002/135-03:33:00 -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Wed May 15 22:36:48 2002 Date: Wed, 8 May 2002 14:28:19 -0700 (PDT) From: Aseel Anabtawi To: len@nova.stanford.edu, hinson@rocc.stanford.edu, rsimpson@magellan.stanford.edu, joe@nova.stanford.edu Cc: Sami.W.Asmar@jpl.nasa.gov, kusza@magellan.stanford.edu Subject: Maneuvers Affecting RS Hello, A mini-sequence is being designed for this weekend that includes maneuvers for MOC calibration. The maneuvers will affect Radio Science in 3 orbits. Our measurements will still be scheduled (turn telemetry off, fix sub-reflector ... etc), but the maneuvers will turn the s/c away from earth around 20 seconds before ingress. The affected orbits are 14194, 14206 and 14222 in sequence mm177. The sequence team would like to know if we are OK with that. If we're not, it is possible to rebuild the whole mini-sequence, but it will take a lot of effort. Please let me know. Regards, Aseel -------------------------------------------------------------------------- From rsimpson@magellan.stanford.edu Wed May 15 22:36:56 2002 Date: Wed, 8 May 2002 14:38:21 -0700 (PDT) From: Dick Simpson 723-3525 To: aseel@godzilla.jpl.nasa.gov, hinson@rocc.stanford.edu, joe@nova.stanford.edu, len@nova.stanford.edu, rsimpson@magellan.stanford.edu Cc: Sami.W.Asmar@jpl.nasa.gov, kusza@magellan.stanford.edu Subject: Re: Maneuvers Affecting RS >The sequence team would like to know if we are OK with that. If >we're not, it is possible to rebuild the whole mini-sequence, but >it will take a lot of effort. Please let me know. I won't vote on whether we can absorb the loss of three occultations; but it sounds as though that's exactly what will happen -- unless they are going to keep the HGA on Earth point while the spacecraft turns, and that seems unlikely. From my own point of view, this might be a good opportunity to check the HGA pointing and pattern. Can we get details on the maneuver, such as where the HGA beam goes during those 20 seconds? How about adding a mini-AZCAL (cross-hair) by taking a couple minutes rather than just 20 secs? We won't get much out of the occultations, I don't think. How can the sequence team be DESIGNING a mini-sequence only four days before they execute that completely reorients the spacecraft? When we've planned bistatic experiments, everything had to be fixed weeks in advance ... -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Wed May 15 22:37:01 2002 Date: Wed, 8 May 2002 15:46:58 -0700 (PDT) From: Aseel Anabtawi To: len@nova.stanford.edu, hinson@rocc.stanford.edu, rsimpson@magellan.stanford.edu, joe@nova.stanford.edu Cc: Sami.W.Asmar@jpl.nasa.gov, kusza@magellan.stanford.edu Subject: Re: Maneuvers Affecting RS Dave, > Losing a few occultations is not a big deal. But we should remind > the sequence team to try to avoid conflicts between occultation > measurements and special maneuvers. In this case the project might > compensate for our loss by requesting extra DSN coverage. What do > you think? If you mean requesting extra DSN coverage this weekend, then it's too late to do that. If you mean in the future, it sounds like a reasonable request to me. However, MGS is already getting more coverage than required, so it may be difficult to ask for more. I did ask the sequence team to try to avoid such conflicts in the future. I was told that such maneuvers are scheduled every six months, and there were some back in October, but I don't remember hearing about them. Pauline Hwang from the sequence team was the one who noticed the conflict when she was reviewing the sequence, and she brought it to my attention. She said that the sequence team is more aware now of what affects Radio Science, so they'll try avoid conflicts or at least let us know about them more in advance. Thank you for willing to give up the three measurements this time. Dick, > I won't vote on whether we can absorb the loss of three > occultations; but it sounds as though that's exactly what > will happen -- unless they are going to keep the HGA on > Earth point while the spacecraft turns, and that seems > unlikely. Pauline checked with Steve Odiorne and he said that the HGA will be set to auto track and it should stay on Earth point during the maneuvers, so it sounds like we will get the entire measurements. The HGA will start turning with the s/c after ingress. > From my own point of view, this might be a good opportunity > to check the HGA pointing and pattern. Can we get details > on the maneuver, such as where the HGA beam goes during > those 20 seconds? How about adding a mini-AZCAL (cross-hair) > by taking a couple minutes rather than just 20 secs? We > won't get much out of the occultations, I don't think. The sequence is not out yet, so I don't have details. Pauline checked with LMA about changing the timing of the maneuvers, and it will take a lot of work at this point. However, she said that we may be able to do that the next time around (in 6 months) if things are planned ahead of time. > How can the sequence team be DESIGNING a mini-sequence only > four days before they execute that completely reorients the > spacecraft? When we've planned bistatic experiments, > everything had to be fixed weeks in advance ... I guess they are not designing it from scratch today, but are in the process of completing the design. They are also using a standard design that was used six months ago when such maneuvers were planned, so it's not entirely new. Regards, Aseel -------------------------------------------------------------------------- From rsimpson@magellan.stanford.edu Wed May 15 22:37:06 2002 Date: Wed, 8 May 2002 17:06:43 -0700 (PDT) From: Dick Simpson 723-3525 To: aseel@godzilla.jpl.nasa.gov, hinson@rocc.stanford.edu, joe@nova.stanford.edu, len@nova.stanford.edu, rsimpson@magellan.stanford.edu Cc: Sami.W.Asmar@jpl.nasa.gov, kusza@magellan.stanford.edu Subject: Re: Maneuvers Affecting RS >Pauline checked with Steve Odiorne and he said that the HGA will be set >to auto track and it should stay on Earth point during the maneuvers, so >it sounds like we will get the entire measurements. The HGA will start >turning with the s/c after ingress. I agree. The only question now is how well the HGA stays on Earth point. There may be some issues in reconstructing the HGA pointing, since the nominal gimbal sampling is only once every 32 sec; but the radio data may not be badly affected. >The sequence is not out yet, so I don't have details. Pauline checked >with LMA about changing the timing of the maneuvers, and it will take >a lot of work at this point. However, she said that we may be able to >do that the next time around (in 6 months) if things are planned ahead >of time. Thorwing in a mini-AZCAL makes no sense if the HGA stays on Earth point (or tries to). >I guess they are not designing it from scratch today, but are in the >process of completing the design. They are also using a standard design >that was used six months ago when such maneuvers were planned, so it's >not entirely new. Sounds like a case of shaping the arguments to fit the desired result. But I'll be quiet now. -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Wed May 15 22:37:15 2002 Date: Wed, 15 May 2002 13:16:21 -0700 (PDT) From: Aseel Anabtawi To: kusza@magellan.stanford.edu Cc: rsimpson@magellan.stanford.edu Subject: Re: Maneuvers Affecting RS > I don't think I saw a 14222i come through, I'm assuming that's ok and it > was not captured on any of the DOY 134 passes. Your assumption is correct. There was no station coverage during this measurement. -------------------------------------------------------------------------- From aseel@godzilla.jpl.nasa.gov Wed May 15 09:32:14 2002 Received: from godzilla.jpl.nasa.gov (godzilla.jpl.nasa.gov [137.78.177.120]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id g4F1s6J25296; Tue, 14 May 2002 18:54:06 -0700 (PDT) Received: from localhost (localhost [127.0.0.1]) by godzilla.jpl.nasa.gov (8.9.3/8.9.3) with SMTP id SAA09338; Tue, 14 May 2002 18:54:53 -0700 (PDT) Message-Id: <200205150154.SAA09338@godzilla.jpl.nasa.gov> Date: Tue, 14 May 2002 18:54:53 -0700 (PDT) From: Aseel Anabtawi Reply-To: Aseel Anabtawi Subject: New RSR Software To: rsimpson@magellan.stanford.edu, joe@nova.stanford.edu, SAbbate@jftl.jpl.nasa.gov Cc: len@nova.stanford.edu, Sami.W.Asmar@jpl.nasa.gov, kusza@magellan.stanford.edu MIME-Version: 1.0 Content-Type: TEXT/plain; charset=us-ascii Content-MD5: qsHIj6YPuLzujI9zmd20BA== X-Mailer: dtmail 1.2.1 CDE Version 1.2.1 SunOS 5.6 sun4u sparc Content-Length: 2591 Hello, The new RSR software was installed on RSR1 at all complexes. It will be installed on RSR2 once we are ready. - The sooner we switch RSR2 to the new software, the better. However, we first need to make sure that there are no problems with RSR1 data. - June 5th is Cassini's month long Solar Conjunction Experiment (SCE). Cassini RS will be using RSR1 at all complexes (RSR1 and RSR3 at SPC-10). We should try to upgrade RSR2 and test before Cassini's SCE when I'll have to free up RSR1. - We need to allow for about a week of testing (parallel RSR1 and RSR2 data) after RSR2 is upgraded. - Starting this week, I will be collecting data on both RSR1 and RSR2, but will only playback RSR1 data. RSR2 data will be saved as backup for a few days in case there are problems with RSR1 data. - When the software is installed, the disk will be wiped out, so any data files that are on the RSRs will be deleted. We need to make sure that we have all RSR2 data before the installation. - VLBI will be using the RSRs at SPC-10 and SPC-40 on 5/18, 5/24, 5/28. Both RSR1 and RSR2 need to be operational on those days so that they use 1, and we use 2. - Our group is moving to another building. The move will start this weekend, and the plan is to move the operations area sometime next week. I wouldn't want the upgrade to happen at the same time the ops machines are being moved. That moves the upgrade to the week after next. With VLBI using one RSR on the 28th, the earlier date for an upgrade that week is the 29th! - Waiting until the 29th gives us a chance to collect RSR1 (new software) data over all complexes, and gives Joe some time to process them using next week's reconstructed SPK file. (Joe, sounds good?) We will also have exactly a week before Cassini's SCE to test RSR2 (with the upgrade) date. Sal, is that cutting it too short? The Cassini group won't be affected by the upgrade as long as they have RSR1 back in time for their SCE. - Cassini RS would like to cleanup the RS TDS and remove unnecessary data files before their SCE. The files on the RS TDS do not get deleted until we (RS) give the OK (this was not the case with the old TDS prior to November of last year). Please let me know if I should keep certain MGS data files. There maybe files there now that are months old, so we can request that files that are over a week (or more?) old be removed. Any comments, questions or suggestions? I know that Dick is away until the 17th, so I don't expect a response from him before then. Regards, Aseel -------------------------------------------------------------------------- From SAbbate@jftl.jpl.nasa.gov Mon May 20 10:17:17 2002 Received: from jftl-mm.jpl.nasa.gov (jftl.jpl.nasa.gov [128.149.117.25]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id g4KHHGW09967 for ; Mon, 20 May 2002 10:17:17 -0700 (PDT) Received: from jftl.jpl.nasa.gov (not verified[128.149.117.23]) by jftl-mm.jpl.nasa.gov with MailMarshal (4,2,5,0) id ; Mon, 20 May 2002 10:18:31 -0700 Received: by JFTL with Internet Mail Service (5.5.2653.19) id ; Mon, 20 May 2002 10:18:09 -0700 Message-ID: <12373B687CF8324F843BE0CA103AA6F41DB778@JFTL> From: "Abbate, Salvatore F" To: rsimpson@magellan.stanford.edu Cc: "Anabtawi, Aseel" Subject: RSR Software DSI-6073-OP-B/3.2 Date: Mon, 20 May 2002 10:18:08 -0700 MIME-Version: 1.0 X-Mailer: Internet Mail Service (5.5.2653.19) Content-Type: text/plain; charset="iso-8859-1" Content-Length: 1685 Status: R Hi Dick The following stations installed DSI 6073-OP-B Ver 3.2 on RSR1 SPC-10 DOY 134 1422 GMT SPC-40 DOY 134 0040 GMT SPC-60 DOY 134 1400 GMT Regards , Sal ACTION JFTL / S ABBATE FROM CAN OPS / L RICARDO / L GEORGE SUBJECT RSR Software DSI-6073-OP-B/3.2 REFERENCE CAD-RS-RSR-013, dated 10 May 2002 CDSCC advises that subject software entered SOAK on DOY134 at 0040z. Regards Leanne George >Starting this week, I will be collecting data on both RSR1 and RSR2, >but will only playback RSR1 data. RSR2 data will be saved as backup >for a few days in case there are problems with RSR1 data. For the record, do you know when the RSR1 software was upgraded at each SPC? >VLBI will be using the RSRs at SPC-10 and SPC-40 on 5/18, 5/24, 5/28. >Both RSR1 and RSR2 need to be operational on those days so that they >use 1, and we use 2. So we go back to old software on those dates. >Cassini RS would like to cleanup the RS TDS and remove unnecessary >data files before their SCE. The files on the RS TDS do not get deleted >until we (RS) give the OK (this was not the case with the old TDS prior >to November of last year). Please let me know if I should keep certain >MGS data files. There maybe files there now that are months old, so we >can request that files that are over a week (or more?) old be removed. I'm not aware of any old data that we would need. As long as we have time to collect the recent data before anything is erased, we should be OK. >Our group is moving to another building ... Didn't realize this. Do you have a new M/S? -------------------------------------------------------------------------- From joe@nova.stanford.edu Thu May 23 14:01:22 2002 Received: from nova.Stanford.EDU (nova [171.64.90.123]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id g4NL1MW00034 for ; Thu, 23 May 2002 14:01:22 -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 OAA00378; Thu, 23 May 2002 14:01:22 -0700 (PDT) Received: from neptune.Stanford.EDU (joe@localhost) by neptune.Stanford.EDU (8.11.6/8.11.6) with ESMTP id g4NKwm709241; Thu, 23 May 2002 13:58:48 -0700 (PDT) Message-Id: <200205232058.g4NKwm709241@neptune.Stanford.EDU> X-Authentication-Warning: neptune.Stanford.EDU: joe owned process doing -bs X-Mailer: exmh version 2.0.2 2/24/98 From: Joe Twicken To: hinson@nova.stanford.edu, joe@nova.stanford.edu, rsimpson@nova.stanford.edu Subject: Re: RSR Notice: /users/z08/procRSR/21430032 In-reply-to: Your message of "Wed, 22 May 2002 17:59:44 PDT." <200205230059.g4N0xig13918@magellan.stanford.edu> References: <200205230059.g4N0xig13918@magellan.stanford.edu> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Date: Thu, 23 May 2002 13:58:48 -0700 Content-Length: 1385 Status: RO (1) There was no HGA motion compensation for these recordings >21340152.RSR p 25XR1IRXN101 25XR1IC1XX01 25XR1IF1S101 25XR1IS1T101 25XR1IS1T201 25XR1IS1T301 25XR1IS1T401 25XR1IS1T501 >21340350.RSR p 25XR1IRXN101 25XR1IC1XX01 25XR1IF1S101 25XR1IS1T101 25XR1IS1T201 25XR1IS1T301 25XR1IS1T401 25XR1IS1T501 >2134035A.RSR p 45XR1IRXN101 45XR1IC1XX01 45XR1IF1S101 45XR1IS1T101 45XR1IS1T201 45XR1IS1T301 45XR1IS1T401 45XR1IS1T501 >21340548.RSR p 45XR1IRXN101 45XR1IC1XX01 45XR1IF1S101 45XR1IS1T101 45XR1IS1T201 45XR1IS1T301 45XR1IS1T401 45XR1IS1T501 >21341339.RSR p 54XR1IRXN101 54XR1IC1XX01 54XR1IF1S101 54XR1IS1T101 54XR1IS1T201 54XR1IS1T301 54XR1IS1T401 54XR1IS1T501 >2134133J.RSR p 65XR1IRXN101 65XR1IC1XX01 65XR1IF1S101 65XR1IS1T101 65XR1IS1T201 65XR1IS1T301 65XR1IS1T401 65XR1IS1T501 >21341536.RSR p 65XR1IRXN101 65XR1IC1XX01 65XR1IF1S101 65XR1IS1T101 65XR1IS1T201 65XR1IS1T301 65XR1IS1T401 65XR1IS1T501 >21341734.RSR p 65XR1IRXN101 65XR1IC1XX01 65XR1IF1S101 65XR1IS1T101 65XR1IS1T201 65XR1IS1T301 65XR1IS1T401 65XR1IS1T501 >21341932.RSR p 65XR1IRXN101 65XR1IC1XX01 65XR1IF1S101 65XR1IS1T101 65XR1IS1T201 65XR1IS1T301 65XR1IS1T401 65XR1IS1T501 >21342130.RSR p 24XR1IRXN101 24XR1IC1XX01 24XR1IF1S101 24XR1IS1T101 24XR1IS1T201 24XR1IS1T301 24XR1IS1T401 24XR1IS1T501 >21342327.RSR p 24XR1IRXN101 24XR1IC1XX01 24XR1IF1S101 24XR1IS1T101 24XR1IS1T201 24XR1IS1T301 24XR1IS1T401 24XR1IS1T501 -------------------------------------------------------------------------- From joe@nova.stanford.edu Fri Nov 15 20:08:35 2002 Received: from nova.Stanford.EDU (nova [171.64.90.123]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id gAG48ZF22497 for ; Fri, 15 Nov 2002 20:08:35 -0800 (PST) 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 UAA23559; Fri, 15 Nov 2002 20:09:00 -0800 (PST) Received: from neptune.Stanford.EDU (joe@localhost) by neptune.Stanford.EDU (8.11.6/8.11.6) with ESMTP id gAG48xQ20426; Fri, 15 Nov 2002 20:08:59 -0800 (PST) Message-Id: <200211160408.gAG48xQ20426@neptune.Stanford.EDU> X-Authentication-Warning: neptune.Stanford.EDU: joe owned process doing -bs X-Mailer: exmh version 2.5 07/13/2001 with nmh-1.0.4 From: Joe Twicken To: hinson@nova.stanford.edu, joe@nova.stanford.edu, rsimpson@nova.stanford.edu Subject: Re: RSR Notice: /users/z15/procRSR/23191852 In-reply-to: Your message of "Fri, 15 Nov 2002 11:20:46 PST." <200211151920.gAFJKkE28272@magellan.stanford.edu> References: <200211151920.gAFJKkE28272@magellan.stanford.edu> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Date: Fri, 15 Nov 2002 20:08:59 -0800 Content-Length: 1829 Status: RO (1) Reprocessed with Goddard trajectory (2) The following recordings were possibly contaminated by momentum desaturations: 21341339.RSR: desaturation from 2002/134-13:11:45.000 to 2002/134-13:14:09.000 2134133J.RSR: desaturation from 2002/134-13:11:45.000 to 2002/134-13:14:09.000 Note that the one-way light time was approximately 20:07 on the date of the recording (3) There was no HGA motion compensation for these recordings >21340152.RSR p 25XR1IRXN102 25XR1IC1XX02 25XR1IF1S102 25XR1IS1T102 25XR1IS1T202 25XR1IS1T302 25XR1IS1T402 25XR1IS1T502 >21340350.RSR p 25XR1IRXN102 25XR1IC1XX02 25XR1IF1S102 25XR1IS1T102 25XR1IS1T202 25XR1IS1T302 25XR1IS1T402 25XR1IS1T502 >2134035A.RSR p 45XR1IRXN102 45XR1IC1XX02 45XR1IF1S102 45XR1IS1T102 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502 >21340548.RSR p 45XR1IRXN102 45XR1IC1XX02 45XR1IF1S102 45XR1IS1T102 45XR1IS1T202 45XR1IS1T302 45XR1IS1T402 45XR1IS1T502 >21341339.RSR p 54XR1IRXN102 54XR1IC1XX02 54XR1IF1S102 54XR1IS1T102 54XR1IS1T202 54XR1IS1T302 54XR1IS1T402 54XR1IS1T502 >2134133J.RSR p 65XR1IRXN102 65XR1IC1XX02 65XR1IF1S102 65XR1IS1T102 65XR1IS1T202 65XR1IS1T302 65XR1IS1T402 65XR1IS1T502 >21341536.RSR p 65XR1IRXN102 65XR1IC1XX02 65XR1IF1S102 65XR1IS1T102 65XR1IS1T202 65XR1IS1T302 65XR1IS1T402 65XR1IS1T502 >21341734.RSR p 65XR1IRXN102 65XR1IC1XX02 65XR1IF1S102 65XR1IS1T102 65XR1IS1T202 65XR1IS1T302 65XR1IS1T402 65XR1IS1T502 >21341932.RSR p 65XR1IRXN102 65XR1IC1XX02 65XR1IF1S102 65XR1IS1T102 65XR1IS1T202 65XR1IS1T302 65XR1IS1T402 65XR1IS1T502 >21342130.RSR p 24XR1IRXN102 24XR1IC1XX02 24XR1IF1S102 24XR1IS1T102 24XR1IS1T202 24XR1IS1T302 24XR1IS1T402 24XR1IS1T502 >21342327.RSR p 24XR1IRXN102 24XR1IC1XX02 24XR1IF1S102 24XR1IS1T102 24XR1IS1T202 24XR1IS1T302 24XR1IS1T402 24XR1IS1T502