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 1998/077." END_OBJECT = TEXT END From trish@rodan.jpl.nasa.gov Tue Mar 17 18:52:47 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 SAA29963 for ; Tue, 17 Mar 1998 18:52:47 -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 SAA02370; Tue, 17 Mar 1998 18:52:39 -0800 (PST) Message-Id: <199803180252.SAA02370@rodan.Jpl.Nasa.Gov> Date: 17 Mar 98 18:55:06 -0800 From: Trish Priest Subject: Occultation #79, Orbit 182 To: David Hinson , Richard Simpson , Joe Twicken , Len Tyler CC: Salvadore Abbate , Sami Asmar , Jennifer Caetta , Paula Eshe , Randy Herrera X-Mailer: QuickMail Pro 1.0.2d1 X-Priority: 3 Reply-To: Trish Priest Content-Type: text/plain; charset="iso-8859-1" Content-Length: 444 Status: O Hello, Occultation 79 went well except that the station had CONSCAN on. Record Times: 077-02:11:00 to 077-02:30:00 One-way Times: 077-02:11:36 to 077-02:29:23 Expected Surface Begin: 077-02:24:22 Expected Eclipse Begin: 077-02:28:34 SNT: 37.37 SPK: spk_i_980317_OD182_192_V1 SOE: p182a.01.soe Script: 98077.34.a182.scr There were no attenuation changes. The next occultation occurs at 7:01 AM PST Wednesday at DSS 65. -Trish ------------------------------------------------------------------------ From pmeshe@mail1.jpl.nasa.gov Wed Mar 18 07:09:58 1998 Received: from eis-msg-002.jpl.nasa.gov (eis-msg-002.jpl.nasa.gov [137.78.160.158]) by magellan.Stanford.EDU (8.8.5/8.8.3) with ESMTP id HAA00443 for ; Wed, 18 Mar 1998 07:09:58 -0800 (PST) Received: from [128.149.43.45] by eis-msg-002.jpl.nasa.gov (Netscape Mail Server v2.02) with ESMTP id AAA7921; Wed, 18 Mar 1998 07:09:58 -0800 Message-Id: Mime-Version: 1.0 Content-Type: text/plain; charset="us-ascii" To: Jen Caetta , Asmar , Salvatore Abbate , Patricia Priest , hinson@nimbus.Stanford.EDU, len@nova.Stanford.EDU, joe@neptune.Stanford.EDU, rsimpson@magellan.stanford.edu From: pmeshe@mail1.jpl.nasa.gov (Paula M Eshe) Subject: Occultation #80 Orbit 183 Date: Wed, 18 Mar 1998 07:09:58 -0800 Content-Length: 386 Status: O Hello Everything went well with Occultation #80 at DSS 65. Record times: 077/14:47:00 to 077/15:06:00 One-way times: 077/14:47:13 to 077/15:05:00 Expected Surface: 077/15:00:00 Expected Eclipse: 077/15:04:11 SNT: 29.50 SOE: p183a.01.soe SPK: spk_i_980317_OD183_193_V1 Script: 98077.65.a183.scr No attenuation changes. The next Occultation occurs at 7:31 PM PST at DSS 34. Paula ------------------------------------------------------------------- From joe@nova.Stanford.EDU Wed Mar 18 10:05:15 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 KAA02617 for ; Wed, 18 Mar 1998 10:05:15 -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 KAA07907; Wed, 18 Mar 1998 10:05:13 -0800 (PST) Received: (from joe@localhost) by neptune.Stanford.EDU (8.8.5/8.8.3) id KAA14797; Wed, 18 Mar 1998 10:00:47 -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: <199803181801.KAA02410@magellan.Stanford.EDU> Date: Wed, 18 Mar 1998 10:00:47 -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/80771758 Content-Length: 236 Status: RO This was the occultation when CONSCAN was on. There are cyclic amplitude fluctuations but the frequency residuals look okay. On 18-Mar-98 Joe Twicken 723-3597 wrote: > 80770211.ODR p 34XRXIR1R201 34XRXIC1XX01 34XR1IF1S101 34XR1IS1T101 ------------------------------------------------------------------- From joe@nova.Stanford.EDU Thu Mar 19 10:05:21 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 KAA20734 for ; Thu, 19 Mar 1998 10:05:21 -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 KAA09810; Thu, 19 Mar 1998 10:05:20 -0800 (PST) Received: (from joe@localhost) by neptune.Stanford.EDU (8.8.5/8.8.3) id KAA15442; Thu, 19 Mar 1998 10:00:53 -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: <199803191803.KAA20657@magellan.Stanford.EDU> Date: Thu, 19 Mar 1998 10:00:52 -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/80781759 Content-Length: 170 Status: RO Sawtooth problem #7. Amplitude of sawtooth is ~1.5 Hz p-p. On 19-Mar-98 Joe Twicken 723-3597 wrote: > 80771447.ODR p 65XRXIR1R201 65XRXIC1XX01 65XR1IF1S101 65XR1IS1T101 ------------------------------------------------------------------- From joe@nova.Stanford.EDU Thu Mar 19 14:31:49 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 OAA24429 for ; Thu, 19 Mar 1998 14:31:48 -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 OAA16785; Thu, 19 Mar 1998 14:31:46 -0800 (PST) Received: (from joe@localhost) by neptune.Stanford.EDU (8.8.5/8.8.3) id OAA15602; Thu, 19 Mar 1998 14:27:14 -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 Date: Thu, 19 Mar 1998 14:27:14 -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, len@nova.Stanford.EDU, trish@zygra.jpl.nasa.gov Subject: USO Allan Deviation: Occultation #77 Content-Length: 594 Status: RO Hello all- I have estimated the USO Allan Deviation for the (approximately) 9.6 minute period of the occultation #79 recording prior to the beginning of the atmospheric occultation. The data were recorded at DSS 34 on 1998/077. The SNR was 50 dB/Hz. t (sec) AD ------- ---------- 0.4096 1.5957e-12 1.6384 6.6810e-13 3.7268 4.7066e-13 6.5536 3.7779e-13 26.2144 2.5537e-13 Note that there are not very many samples from which to estimate Allan Deviation at the longest integration time. Joe