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 1997/336." END_OBJECT = TEXT END From trish@rodan.jpl.nasa.gov Tue Dec 2 15:32:28 1997 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 PAA07658 for ; Tue, 2 Dec 1997 15:32:28 -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 PAA27266; Tue, 2 Dec 1997 15:32:33 -0800 (PST) Message-Id: <199712022332.PAA27266@rodan.Jpl.Nasa.Gov> Date: 02 Dec 97 15:36:33 -0800 From: Trish Priest Subject: RE: ingress timing To: Dave Hinson CC: len , rsimpson X-Mailer: QuickMail Pro 1.0.2d1 X-Priority: 3 Reply-To: Trish Priest Content-Type: text/plain; charset="iso-8859-1" Content-Length: 2188 Status: RO I also added one more selling point -- the distinct lack of occultations during any proposed phasing orbit. -Trish Dave Hinson wrote: >Trish, > >I agree -- let's plan to ask for -10 to +2 minutes and see how >people react. The exception is in late January, when the spacecraft >is not yet occulted by Mars' surface. Dick would like to see some >data during these highly grazing occultations to look for scattering >from the surface. Best to check with him in formulating a strategy >for collecting data. > >Your question about the turn-around time for profiles is a very good >one. Our ability to provide unique information to the Atmospheric >Advisory Group is a strong selling point. Once the raw data and SPK >files are in our hands, data analysis should take no more than a few >days initially, and less than one day after some practice. This will >be a challenge, however, because we're reducing our budgets for the >current fiscal year so as to better stretch our funding into the delayed >mapping phase. > >Here is the list of selling points, with some minor changes. > >Thanks, >Dave > >------------------------ > >1. On the HGA, the RST would obtain high quality occultation data -- >approximately 100 times better than the data collected at MOI and 100 >times better than Viking data. > >2. These data would be collected at Southern Summer over a wide range >of latitudes (40 deg N to 65 deg S). The data will provide a "snapshot" >of the atmosphere during a single season. Occultation latitude slews >from 40 deg N to 65 deg S in about 40 days. > >3. About 300 occultations would be observed in a period of 4 months. > >4. The experiments would provide atmospheric data when the other >instruments are turned off. Information would be for a specific latitude >that is generally not close to periapsis on the same orbit. However, the >measurements could detect substantial dust storms if they occur. > >5. This series of experiments would put the Radio Science open-loop >equipment, remote operations, and the support team through operations >resembling mapping -- before our remote operations developer leaves JPL.