PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM DATA_SET_ID = "MEX-M-MRS-1/2/3-NEV-0005-V1.0" STANDARD_DATA_PRODUCT_ID = ENB PRODUCER_ID = "SUE" PRODUCT_ID = "M00SUE0L1A_ENB_031871418_00.TXT" PRODUCT_CREATION_TIME = 2006-06-28T17:49:24.000 INSTRUMENT_HOST_ID = "MEX" OBJECT = TEXT PUBLICATION_DATE = 2005-02-12 NOTE = "MEX SUE Experimenter Notes" END_OBJECT = TEXT END From paetzold.martin@web.de Wed Jul 2 00:16:49 2003 Received: from mailgate5.cinetic.de (mailgate5.cinetic.de [217.72.192.165]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id h627Gm802795 for ; Wed, 2 Jul 2003 00:16:48 -0700 (PDT) Received: from web.de (fmomail02.dlan.cinetic.de [172.20.1.46]) by mailgate5.cinetic.de (8.11.6p2/8.11.2/SuSE Linux 8.11.0-0.4) with SMTP id h627GRQ01646; Wed, 2 Jul 2003 09:16:27 +0200 Date: Wed, 2 Jul 2003 09:16:27 +0200 Message-Id: <200307020716.h627GRQ01646@mailgate5.cinetic.de> MIME-Version: 1.0 Organization: http://freemail.web.de/ From: =?iso-8859-1?Q?"Martin=20P=E4tzold"?= To: bernd.haeusler@unibw-muenchen.de, hagerman@geo.uni-koeln.de, len.tyler@stanford.edu, rsimpson@magellan.stanford.edu, sami.w.asmar@jpl.nasa.gov Subject: Fwd: NNO operator NO LONGER required for 6th and 10th July Precedence: fm-user Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit Content-Length: 1197 Status: O Peter.Schmitz@esa.int schrieb am 02.07.03 07:21:31: > > Marco, > > the PI gave his o.k to your proposal to configure IFMS-A for X-D/L and IFMS-B > for S-D/L during the Canberra pass on DOY 187 > Hence there is no longer a local operator at NNO required to configure the > IFMS-RS. > > Please find below the updated requirements: > > During the Canberra passes: > > Sunday 06/07/03 Radio Science (One Way Dual D/L @ CAN+NNO) > IFMS-A : X-D/L-CL; smpl rate = 1 smpl/s > IFMS-B : S-D/L-CL; smpl rate = 1 smpl/s > IFMS-RS: no required > Recording and data routing to DDS of: > - Doppler Data [1 smpl/s] > - Meteo Data [1 smpl/min] > - AGC Data [1 smpl/s] > > After the Canberra pass: > After the Canberra passes configure IFMS-A for X-U/L and reconfigure IFMS-B for > X-D/L to maintain the redundancy. > > > Thursday 10/07/03 Radio Science (One Way Single D/L @ CAN+NNO) > IFMS-A : X-D/L-CL; smpl rate = 1 smpl/s > IFMS-B : X-D/L-CL; smpl rate = 1 smpl/s > IFMS-RS: not required > Recording and data routing to DDS of: > - Doppler Data [1 smpl/s] > - Meteo Data [1 smpl/min] > - AGC Data [1 smpl/s] > > After the Canberra pass: > After the Canberra passes configure IFMS-A for X-U/L - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Received: from methusalix.geo.Uni-Koeln.DE (methusalix.geo.Uni-Koeln.DE [134.95.160.200]) by pluto.geo.Uni-Koeln.DE (8.12.8/8.12.8) with ESMTP id h649lZMc015316 for ; Fri, 4 Jul 2003 11:47:35 +0200 (MET DST) Received: from esacom59-int.esoc.esa.int (esacom59-ext.esoc.esa.int [131.176.86.4]) by methusalix.geo.Uni-Koeln.DE (8.11.6/8.11.3) with ESMTP id h649lYo27182 for ; Fri, 4 Jul 2003 11:47:35 +0200 (MEST) Received: from esacom53.esoc.esa.de (esacom53.esoc.esa.int [131.176.85.6]) by esacom59-int.esoc.esa.int (8.12.9/8.12.9/ESA-External-v3.2) with ESMTP id h649lTtj007071 for ; Fri, 4 Jul 2003 11:47:29 +0200 (MET DST) Received: from esocmail2.esoc.esa.int (esocmail2.esoc.esa.int [131.176.51.225]) by esacom53.esoc.esa.de (8.12.9/8.12.9/ESA-Internal-v3.2) with SMTP id h649lTSC014809 for ; Fri, 4 Jul 2003 09:47:29 GMT Received: by esocmail2.esoc.esa.int(Lotus SMTP MTA v4.6.7 (934.1 12-30-1999)) id 41256D59.003BA533 ; Fri, 4 Jul 2003 11:51:29 +0100 X-Lotus-FromDomain: ESA From: John.Reynolds@esa.int To: Peter.Schmitz@esa.int cc: Marco.Lanucara@esa.int, Justin.Howard@esa.int, Juergen.Fay@esa.int, Michel.Denis@esa.int, Esoc.SCHEDOD@esa.int, Alan.Moorhouse@esa.int, paetzold@geo.Uni-Koeln.DE Message-ID: <41256D59.003BA4CC.00@esocmail2.esoc.esa.int> Date: Fri, 4 Jul 2003 10:47:19 +0100 Subject: Re: NNO operations over the coming weekend Mime-Version: 1.0 Content-type: text/plain; charset=us-ascii Content-Disposition: inline X-Mozilla-Status2: 00000000 Dear All, we have a problem with IFMS1 Meteo sensor. This means that for the weekend IFMS2 will be prime for uplink activities. Regards John |--------+-----------------------> | | Peter Schmitz| | | | | | 2003-07-01 | | | 21:51 | | | | |--------+-----------------------> >----------------------------------------------------------------------------| | | | To: Marco Lanucara/esoc/ESA@ESA, Justin Howard/esoc/ESA@ESA, John| | Reynolds/esoc/ESA@ESA | | cc: Juergen Fay/esoc/ESA@ESA, Michel Denis/esoc/ESA@ESA, Esoc | | SCHEDOD/esoc/ESA@ESA, Alan Moorhouse/esoc/ESA@ESA, | | paetzold@geo.Uni-Koeln.DE | | Subject: NNO operator NO LONGER required for 6th and 10th July | >----------------------------------------------------------------------------| Marco, the PI gave his o.k to your proposal to configure IFMS-A for X-D/L and IFMS-B for S-D/L during the Canberra pass on DOY 187 Hence there is no longer a local operator at NNO required to configure the IFMS-RS. Please find below the updated requirements: During the Canberra passes: Sunday 06/07/03 Radio Science (One Way Dual D/L @ CAN+NNO) IFMS-A : X-D/L-CL; smpl rate = 1 smpl/s IFMS-B : S-D/L-CL; smpl rate = 1 smpl/s IFMS-RS: no required Recording and data routing to DDS of: - Doppler Data [1 smpl/s] - Meteo Data [1 smpl/min] - AGC Data [1 smpl/s] After the Canberra pass: After the Canberra passes configure IFMS-A for X-U/L and reconfigure IFMS-B for X-D/L to maintain the redundancy. Thursday 10/07/03 Radio Science (One Way Single D/L @ CAN+NNO) IFMS-A : X-D/L-CL; smpl rate = 1 smpl/s IFMS-B : X-D/L-CL; smpl rate = 1 smpl/s IFMS-RS: not required Recording and data routing to DDS of: - Doppler Data [1 smpl/s] - Meteo Data [1 smpl/min] - AGC Data [1 smpl/s] After the Canberra pass: After the Canberra passes configure IFMS-A for X-U/L - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - From aseel@godzilla.jpl.nasa.gov Sun Jul 6 19:04:11 2003 Received: from godzilla.jpl.nasa.gov (godzilla.jpl.nasa.gov [137.78.78.95]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id h6724A813676 for ; Sun, 6 Jul 2003 19:04:10 -0700 (PDT ) Received: from aseel (aseel.jpl.nasa.gov [137.78.78.43]) by godzilla.jpl.nasa.gov (8.9.3p2.cm/8.9.3) with SMTP id TAA11577; Sun, 6 Jul 2003 19:04:09 -0700 (PDT) Message-ID: <00d501c3442b$fa2bc1c0$2b4e4e89@jpl.nasa.gov> Reply-To: "Aseel Anabtawi" From: "Aseel Anabtawi" To: "Dick Simpson 723-3525" Cc: Subject: MEX Y-factor and more Date: Sun, 6 Jul 2003 19:03:36 -0700 MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="----=_NextPart_000_00D2_01C343F1.4DB51C00" X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Content-Length: 31443 Status: RO This is a multi-part message in MIME format. ------=_NextPart_000_00D2_01C343F1.4DB51C00 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit Hello again, Below are the Y-factor measurements from DSS-43. The Pre-Cal S1 and S2 Y-factor values that are shown here are reversed compared to what Kevin gave me over the voice net (the T-Op values are fine). They are very close, but if you want, I can double check with Kevin that they are correct. DR# C102520 was opened for late AOS. I've saved the details of the DR in the attached document. Lastly, the station went through the whole pre-cal process during post-cal, and not just getting the Y-factor values. Regards, Aseel ----- Original Message ----- From: "Piechowski, Kevin J" Sent: Sunday, July 06, 2003 4:23 PM Subject: DSS43 Y-Factor measurements > Aseel > > G'day. Hows it going. The results for DSS43 MEX Radio Science Y-Factor > measurements are as follows > > Precal > > Y-Factor T-Op > > X1 12.618 16.378 > X2 12.347 17.349 > S1 10.66 25.373 > S2 10.62 25.971 > > Postcal > > X1 12.773 15.861 > X2 12.589 16.533 > S1 12.948 14.983 > S2 10.649 25.753 > > There is a discrepency with the S1 pre & post cal. We were pushed for time > to investigate this but we will be able to check this during tomorrows > maintenance period. > Measurements were performed utilising the LNA instrumentation rack. > > Regards KJP ------=_NextPart_000_00D2_01C343F1.4DB51C00 Content-Type: application/msword; name="MEX_DR_C102520.doc" Content-Transfer-Encoding: base64 Content-Disposition: attachment; filename="MEX_DR_C102520.doc" ... - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - From Thomas.W.Thompson@jpl.nasa.gov Fri Jul 11 15:02:20 2003 Received: from ampersand.jpl.nasa.gov (ampersand.jpl.nasa.gov [137.78.28.29]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id h6BM2JC07719 for ; Fri, 11 Jul 2003 15:02:19 -0700 (PDT) Received: from [128.149.231.103] (dialin-103.jpl.nasa.gov [128.149.231.103]) by ampersand.jpl.nasa.gov (8.12.9/8.12.8/RSE-2.2) with ESMTP id h6BM00DW024033; Fri, 11 Jul 2003 15:00:02 -0700 (PDT) Mime-Version: 1.0 X-Sender: twt@radar-sci.jpl.nasa.gov@comma.jpl.nasa.gov (Unverified) Message-Id: Date: Fri, 11 Jul 2003 14:59:59 -0700 To: carr@astmnl.wr.usgs.gov, rkirk@usgs.gov, barchinal@usgs.gov, greeley@asu.edu, david.williams@asu.edu, ekolb@cox.net, james_head_III@brown.edu, Harald_Hiesinger@brown.edu, misha@mare.geo.brown.edu, mccordtb@aol.com, squyres@astrosun.astro.cornell.edu, rjs33@cornell.edu, donald-gurnett@uiowa.edu, dlk@space.physics.uiowa.edu, estofan@yahoo.com, ellen@proxemy.com, sandel@arizona.edu, astern@boulder.swri.edu, atreya@umich.edu, ghansen@rad.geology.washington.edu, len@nova.stanford.edu, rsimpson@magellan.stanford.edu, hinson@rocc.stanford.edu, everett.k.gibson@jsc.nasa.gov, arvidson@wunder.wustl.edu, John_Mustard@brown.edu, richard.v.morris@nasa.gov, clifford@lpi.usra.edu, william.farrell@gsfc.nasa.gov, Carl.Leuschen@jhuapl.edu, phillips@wustite.wustl.edu, twatters@nasm.si.edu From: Thomas W Thompson Subject: Mars Express Update - 11 July 03 Content-Type: multipart/alternative; boundary="============_-1154161690==_ma============" Content-Length: 3039 Status: RO --============_-1154161690==_ma============ Content-Type: text/plain; charset="us-ascii" ; format="flowed" Near-Earth Verification (Spacecraft and Instrument/Experiment Commissioning), which commenced on June 16, 2003, continues with personnel at the European Space Operations Centre (ESOC) reporting, "spacecraft platform subsystems and payload behave in a nominal manner". Since last week's report several important tests have been completed. The Payload MARSIS Interference Test was completed on July 3, 2003 with results indicating that spacecraft and/or instrument noise will not affect the MARSIS Measurements experiment once in orbit at Mars. An Earth-Moon photo sequence on July 3, 2003 was successful with acquisition of an HRSC-SRC earth image, OMEGA spectra, SPICAM spectra and PSF spectra. There was successful Beagle2 Turn-on and Checkout on July 4-5, 2003 as described in an ESA press release earlier this week. The first Radio Science test (which simulated bistatic radar data acquisition) with the Deep Space Network 70-meter antenna at Canberra was a success, according to Sami Asmar, Investigation Scientist for Mars Express Radio Science. Four more Radio Science tests with DSN stations are scheduled through Saturday, July 19, 2003. Near-Earth Verification should be completed on July 20, 2003 - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - From rsimpson@airmail.fltops.jpl.nasa.gov Thu Oct 2 17:46:49 2003 Received: from airmail1.fltops.jpl.nasa.gov (airmail2.fltops.jpl.nasa.gov [137.228.96.27]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id h930knx08066 for ; Thu, 2 Oct 2003 17:46:49 -0700 (PDT) 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 4EE471092E for ; Thu, 2 Oct 2003 17:46:45 -0700 (PDT) Received: (from rsimpson@localhost) by rsops2.fltops.jpl.nasa.gov (8.11.6+Sun/8.11.6) id h930kjn13724 for rsimpson@magellan.stanford.edu; Fri, 3 Oct 2003 00:46:45 GMT Date: Fri, 3 Oct 2003 00:46:45 GMT From: Richard A Simpson Message-Id: <200310030046.h930kjn13724@rsops2.fltops.jpl.nasa.gov> To: rsimpson@magellan.stanford.edu Subject: MEX NEVT RSR File List Content-Length: 1683 -rw-r--r-- 1 rssg 8097 81867660 Aug 18 00:13 mex_doy187_dss43_r1a_nx_141830to143200.rsr -rw-r--r-- 1 rssg 8097 2327986860 Aug 26 23:02 mex_doy187_dss43_r1a_nx_154500to220900.rsr -rw-r--r-- 1 rssg 8097 81867660 Aug 19 01:22 mex_doy187_dss43_r1b_ns_141830to143200.rsr -rw-r--r-- 1 rssg 8097 1533938760 Aug 18 23:53 mex_doy187_dss43_r1b_ns_154500to195801.rsr -rw-r--r-- 1 rssg 8097 81867660 Aug 26 22:01 mex_doy187_dss43_r2a_nx_141830to143200.rsr -rw-r--r-- 1 rssg 8097 1627223940 Aug 26 22:39 mex_doy187_dss43_r2a_nx_154500to220900.rsr -rw-r--r-- 1 rssg 8097 81766620 Aug 26 22:31 mex_doy187_dss43_r2b_ns_141831to143200.rsr -rw-r--r-- 1 aseel 8097 260304300 Aug 27 03:03 mex_doy187_dss43_r2b_ns_154500to162756.rsr -rw-r--r-- 1 aseel 8097 1765093020 Aug 27 03:13 mex_doy187_dss43_r2b_ns_162808to211917.rsr -rw-r--r-- 1 rssg 8097 2455297260 Aug 26 23:23 mex_doy191_dss43_r2a_nx_124500to193000.rsr -rw-r--r-- 1 rssg 8097 2128584420 Aug 26 23:39 mex_doy191_dss43_r2b_nx_124500to193000.rsr -rw-r--r-- 1 rssg 8097 147614460 Jul 30 22:51 mex_doy192_dss24_r2b_sx_074110to123900.rsr -rw-r--r-- 1 rssg 8097 49948220 Jul 30 22:46 mex_doy192_dss24_r3b_ss_074100to092146.rsr -rw-r--r-- 1 rssg 8097 97567120 Jul 30 22:34 mex_doy192_dss24_r3b_ss_092209to123900.rsr -rw-r--r-- 1 rssg 8097 15619660 Aug 27 00:08 mex_doy195_dss24_r2b_ss_074400to081530.rsr -rw-r--r-- 1 rssg 8097 196265860 Jul 30 21:40 mex_doy200_dss15_r3a_xx_072400to140000.rsr -rw-r--r-- 1 rssg 8097 183380260 Aug 4 18:42 mex_doy200_dss15_r3b_xs_075000to140000.rsr - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - From aseel@godzilla.jpl.nasa.gov Thu Oct 9 15:29:55 2003 Received: from godzilla.jpl.nasa.gov (godzilla.jpl.nasa.gov [137.78.78.95]) by magellan.stanford.edu (8.11.6/8.11.6) with ESMTP id h99MTtx05925 for ; Thu, 9 Oct 2003 15:29:55 -0700 (PDT) Received: from aseel (aseel.jpl.nasa.gov [137.78.78.43]) by godzilla.jpl.nasa.gov (8.9.3p2.cm/8.9.3) with SMTP id PAA10548 for ; Thu, 9 Oct 2003 15:29:50 -0700 (PDT) Message-ID: <01c001c38eb4$c0ba05e0$2b4e4e89@jpl.nasa.gov> Reply-To: "Aseel Anabtawi" From: "Aseel Anabtawi" To: "Dick Simpson 723-3525" References: <200310080209.h9829Em07066@magellan.stanford.edu> Subject: Re: MEX 187 X/L Test Date: Thu, 9 Oct 2003 15:29:07 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Content-Length: 1301 Status: R > Aseel: > > Do you have any log/summary files to accompany > mex_doy187_dss43_r2a_nx_154500to220900.rsr ? I ran RSRInfo on the file (which is a program that someone in our group wrote, and it displays information about the RSR data file, including gaps) and this is what I got: DATE OF GENERATION: Thu Oct 9 22:22:33 2003 REPORT FOR FILE: mex_doy187_dss43_r2a_nx_154500to220900.rsr Start Time: 2003 187 15:45:00 End Time : 2003 187 22:09:00 Elapsed Time : 23040 seconds Pass No.: 35 Tracking Mode: 1-Way Spacecraft No.: 41 DSS No.: 43 RSR ID: 3 Sub 1 Processing Center: 40 Sample Rate: 25000 per second Sample Resolution: 16 bit Uplink Band: N/A Downlink Band: X First Record Seq. No.: 40 Last Record Seq. No.: 26664 Gaps Found: 2 Data Errors: 0 So, yes, there are gaps. This was *not* one of the two files that I was planning on re-querying (by the way, the data are still on the CDR, but I haven't heard back from DC on whether they processed it or not). The two files are: mex_doy187_dss43_r1b_ns_154500to195801.rsr (should end at 22:09:00) mex_doy187_dss43_r2b_ns_162808to211917.rsr (same as above) > Don't worry about trying to recover lost records. If I can, I will.