PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM DATA_SET_ID = "MEX-M-MRS-1/2/3-EXT2-2601-V1.0" STANDARD_DATA_PRODUCT_ID = ENB PRODUCER_ID = "SUE" PRODUCT_ID = "M00SUE0L1A_ENB_100621849_00.TXT" PRODUCT_CREATION_TIME = 2015-03-20T10:49:04.000 INSTRUMENT_HOST_ID = "MEX" OBJECT = TEXT PUBLICATION_DATE = 2011-03-10 NOTE = "MEX SUE Experimenter Notes" END_OBJECT = TEXT END From Thomas.W.Thompson@jpl.nasa.gov Fri Feb 12 15:53:48 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion2.jpl.nasa.gov [128.149.139.106]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o1CNrmj29267 for ; Fri, 12 Feb 2010 15:53:48 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap02.jpl.nasa.gov [128.149.137.73]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o1CNrgdC025260 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL) for ; Fri, 12 Feb 2010 15:53:49 -0800 Received: from ALTPHYEMBEVSP10.RES.AD.JPL ([172.16.0.11]) by ALTVIREHTSTAP02.RES.AD.JPL ([128.149.137.73]) with mapi; Fri, 12 Feb 2010 15:53:43 -0800 From: "Thompson, Thomas W (3300)" To: "Simpson, Richard A (6520-Affiliate)" Date: Fri, 12 Feb 2010 15:53:41 -0800 Subject: Thanks: Any comments - New posting for ESA MEX Blog - Phobos Fly-by - Thread-Topic: Thanks: Any comments - New posting for ESA MEX Blog - Phobos Fly-by - Thread-Index: AcqsMqW2KfORoFK/Tp2kqDcUNQMMvQAC/SWT Message-ID: In-Reply-To: <201002122228.o1CMS1929117@magellan.stanford.edu> Accept-Language: en-US Content-Language: en X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/alternative; boundary="_000_C79B2A05E109ThomasWThompsonjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap02.jpl.nasa.gov [128.149.137.73] X-Source-Sender: Thomas.W.Thompson@jpl.nasa.gov X-AUTH: Authorized Content-Length: 13117 Status: RO --_000_C79B2A05E109ThomasWThompsonjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable Hi Dick - Many Thanks - Tommy On 2/12/10 2:28 PM, "Dick Simpson 650-723-3525" wrote: >Any comments before I respond back to Daniel on Tuesday ? - Looks OK to me It's a good article. No corrections or changes. If he wants to expand, he could note that the MEX radio science investigators are hoping that the close approach will provide not only much better estimates of Phobos' mass but also how the mass is distributed within the satellite. That is, there appear to be pockets of slightly denser material scattered through Phobos; by passing within 50 km, MEX may respond to those differences and the Doppler measurements will reveal where the denser material hides. There are also two MEX radio science groups working on Phobos. The radio science PI Martin Paetzold and Tom Andert lead one group in Germany; Pascal Rosenblatt leads the other group at the Royal Observatory in Brussels. - - - - - - - - - - - - - - - - - - - - - - - - - - - - From: Date: Fri, 12 Feb 2010 06:37:21 -0800 To: "Thompson, Thomas W" Subject: New posting for ESA MEX Blog Tommy, Daniel Scuka here; I am the editor covering operations for ESA's website, based at ESOC/Darmstadt. The colleagues on the MEX Flight Control Team have kindly sent me some information on the use of DSS-63 for the 3 March MEX-Phobos flyby (for radio science). I have written a short blog post for our new MEX blog (http://www.esa.int/mexblog). I was wondering if you could (a) review the text below to see if I've made any errors, and (b) it would be fantastic if you had time to send me a few sentences and a quote...? I would include this into the final version of the post. Ideally, I'd like to publish this on Monday or tuesday, 15/16 Feb. Many thanks and best regards from cold and snowy Darmstadt, -- Daniel EJR-Quartz for ESA - European Space Agency Daniel Scuka SSA Communication Coordinator Senior Editor for Spacecraft Operations Communication and Knowledge Department ESOC Robert-Bosch-Strasse 5 64293 Darmstadt, Germany daniel.scuka@esa.int | www.esa.int T +49 6151 90 2601 | F +49 6151 90 495 M +49 170 286 3718 Phobos flyby radio science supported by NASA's Big Dish NASA's Deep Space Network (DSN) will play a critical role in the central science activity for the 3 March flyby. The American space agency's giant 70m station at Robledo, Spain (DSS-63), will be enlisted to track ESA's Mars Express during Phobos flyby to record extremely precise Doppler data - which in turn will enable Mars Express scientists to obtain the best-ever measurements of Phobos gravity and hence mass. Yes, ESA's own 'giant' 35m Deep Space Antenna, DSA-2 at Cebreros station, also in Spain, will be involved - for telecommanding, telemetry receipt and as back-up for the radio science tracking. Yes, the flyby could still be done using only ESA's Cebreros station, but the radio science data quality will be greatly improved by the use of the NASA 70m antenna - like listening with a much bigger ear! The practical effect of using the bigger NASA dish is that we'll improve the signal-to-noise ratio - i.e. we'll hear the spacecraft signal more clearly over the background 'noise'. This lets us better detect the subtle changes in the radio signal that will be caused by Phobos. As Mars Express passes Phobos, the Martian moon will change our spacecraft's velocity and this will result in a change in the frequency of the signal sent by Mars Express back to Earth (through the Doppler effect - like the change in tone of an ambulance siren as it passes). "We're grateful to NASA for giving us the time on this dish because there are only three stations like this in the world and they're understandably very busy supporting all sorts of missions in far flung parts of the Solar System," said Michel Denis, Mars Express Spacecraft Operations (SOM) manager here at ESOC. We've posted some Flickr images below taken by Mars Express Spacecraft Operations Engineer (and one of the contributors to this blog!) Thomas Ormston. The first show DSS-63 - one of only three 70m antennas on Earth. After three years of construction, the original antenna (64m) was finished in 1973 to support early JPL Mars missions. In the 1980s, the upgrade to 70m was made to support the Voyager extended mission. http://www.flickr.com/photos/thomas_ormston/sets/72157605571353325/ The next set of images show the MDSCC (Madrid Deep Space Communications Complex) control centre at Robledo - run by Spanish contractor INTA on behalf of NASA. http://www.flickr.com/photos/thomas_ormston/sets/72157605579459793/ Finally, a couple sets showing ESA's own 35m antenna at Cebreros http://www.flickr.com/photos/thomas_ormston/sets/72157605576298784/ ... and the Cebreros Operations Centre http://www.flickr.com/photos/thomas_ormston/sets/72157605581422127/ Like all stations in ESA's global ESTRACK station network, Cebreros is remote-controlled from the ESTRACK Control Centre at ESOC here in Darmstadt; the industrial support engineers on site take care of regular maintenance and do go 'on-console' for critical operations - like Phobos flyby. From Olivier.Reboud@esa.int Mon Feb 15 08:40:47 2010 Return-Path: Received: from esacom90-int.esrin.esa.int (esacom90-ext.esrin.esa.int [192.171.5.18]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o1FGejj02803 for ; Mon, 15 Feb 2010 08:40:46 -0800 (PST) Received: from esacom66.esrin.esa.int (192-171-5-30.esrin.esa.int [192.171.5.30]) by esacom90-int.esrin.esa.int (8.13.3/8.13.3/ESA-External-v4.0) with ESMTP id o1FGed4k002925; Mon, 15 Feb 2010 16:40:39 GMT Received: from esrinmta1.esrin.esa.int (esrinnotesadmin-a.esrin.esa.int [193.204.225.153]) by esacom66.esrin.esa.int (8.12.10/8.12.10/ESA-Internal-v3.2) with ESMTP id o1FGebkn004875; Mon, 15 Feb 2010 16:40:38 GMT To: "Velasco, Jesse" Cc: stefan.remus@sciops.esa.int, Hannes.Griebel@esa.int, John.Reynolds@esa.int, mexmps@esa.int, sami.w.asmar@jpl.nasa.go, julia.l.bell@jpl.nasa.gov, susan.c.kurtik@jpl.nasa.gov, rsimpson@magellan.stanford.edu, Thomas.Ormston@esa.int Subject: Questions for the MEX Phobos flyby Doy062-2010 preparation MIME-Version: 1.0 X-Mailer: Lotus Notes Release 6.5.5 November 30, 2005 Message-ID: From: Olivier.Reboud@esa.int Date: Mon, 15 Feb 2010 17:40:25 +0100 X-MIMETrack: Serialize by Router on esrinmta1/esrin/ESA at 02/15/2010 17:40:38, Serialize complete at 02/15/2010 17:40:38 Content-Type: multipart/alternative; boundary="=_alternative 005B9733C12576CB_=" Content-Length: 1646 Status: RO This is a multipart message in MIME format. --=_alternative 005B9733C12576CB_= Content-Type: text/plain; charset="US-ASCII" Dear Jesse, In the scope of the MEX Phobos flyby Doy062-2010 preparation, do you have a list of the key settings which will be used for DSS-63 receiver in X and S-Band (PLL Loop bandwidth should be set to 25Hz for X-band because of coherent D/L but are there others important settings of the Station Receiver that RS team should know about, like the PLL-Loop Bandwidth used for the coherent S-Band D/L) ? Another question in the same context : At which frequency do you intend to sample the recorded station parameters during the support, and which are the rates available for this sampling ? Best regards, Olivier From jesse.velasco@dsn.nasa.gov Tue Feb 16 11:24:41 2010 Return-Path: Received: from DSNOAM-MM.jpl.nasa.gov (dsnoam-mm.jpl.nasa.gov [128.149.207.83]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o1GJOdj10902 for ; Tue, 16 Feb 2010 11:24:39 -0800 (PST) Received: from dsnoamex1.jpl.nasa.gov (Not Verified[128.149.207.88]) by DSNOAM-MM.jpl.nasa.gov with MailMarshal (v6,4,6,5922) id ; Tue, 16 Feb 2010 11:25:09 -0800 X-MimeOLE: Produced By Microsoft Exchange V6.5 Content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01CAAF3C.C618C0C5" Subject: RE: Questions for the MEX Phobos flyby Doy062-2010 preparation Date: Tue, 16 Feb 2010 11:18:07 -0800 Message-ID: In-Reply-To: X-MS-Has-Attach: X-MS-TNEF-Correlator: Thread-Topic: Questions for the MEX Phobos flyby Doy062-2010 preparation Thread-Index: AcquXby2pPl3OjSxR7qOnvVYhJHzggA1Mx0A References: From: "Velasco, Jesse" To: Cc: , , , , , , , , , "!DL-DSN-MPSETD" , , "Goltz, Gene L" Content-Length: 8469 Status: RO This is a multi-part message in MIME format. ------_=_NextPart_001_01CAAF3C.C618C0C5 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: quoted-printable Olivier, We are going to use our nominal default receiver configuration setting for the Phobos fly-by. The PLL loop bandwidth setting for X-band coherent is 25 Hz and S-band coherent is also 25 Hz. Please advise us of any special setting you may require. Radio Science team uses a dedicated RSR (Radio Science Receiver) and they control their own setting. My understanding is they will use their default settings. Are you referencing tracking data, or Radio Science data when you talk about recorded station parameters? For MEX tracking data we sample 1/60, however, we have the option to sample at 1/10 and 1/1. Radio Science deliver their files at 2kHz.=20 If you need any clarification please let me know. In the future please copy !DL-DSN-MPSETD@dsn.nasa.gov on your email messages to the NOPEs. This will ensure your emails are received by the NOPEs and are answered in a timely manner.=20 Thanks Jesse Velasco MEX NOPE From jesse.velasco@dsn.nasa.gov Tue Feb 16 11:59:51 2010 Return-Path: Received: from mdsccmmwa.mdscc.nasa.gov (mdsccmmwa.mdscc.nasa.gov [198.116.30.6]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o1GJxoj11197 for ; Tue, 16 Feb 2010 11:59:50 -0800 (PST) Received: from mdsccex1.mdscc.nasa.gov (Not Verified[198.116.30.73]) by mdsccmmwa.mdscc.nasa.gov with MailMarshal (v6,4,6,5922) id ; Tue, 16 Feb 2010 21:00:20 +0100 Received: from dsnoamex1.jpl.nasa.gov ([128.149.207.88]) by mdsccex1.mdscc.nasa.gov with Microsoft SMTPSVC(6.0.3790.3959); Tue, 16 Feb 2010 21:00:20 +0100 X-MimeOLE: Produced By Microsoft Exchange V6.5 Content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Subject: RE: Questions for the MEX Phobos flyby Doy062-2010 preparation Date: Tue, 16 Feb 2010 11:58:20 -0800 Message-ID: In-Reply-To: <201002161930.o1GJUNA10926@magellan.stanford.edu> X-MS-Has-Attach: X-MS-TNEF-Correlator: Thread-Topic: Questions for the MEX Phobos flyby Doy062-2010 preparation Thread-Index: AcqvPpyq6Tdru0v4TwK1waLoLyP26wAAnehg References: <201002161930.o1GJUNA10926@magellan.stanford.edu> From: "Velasco, Jesse" To: "Dick Simpson 650-723-3525" X-OriginalArrivalTime: 16 Feb 2010 20:00:20.0384 (UTC) FILETIME=[AAECFA00:01CAAF42] Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by magellan.stanford.edu id o1GJxoj11197 Content-Length: 1013 Status: RO Dick, You are correct. RMDC selects the sample rate and will use the default rate for that project if not instructed to use another sample rate. I forgot to list the sample rate of 10/1. Jesse -----Original Message----- From: Dick Simpson 650-723-3525 [mailto:rsimpson@magellan.stanford.edu] Sent: Tuesday, February 16, 2010 11:30 AM To: Velasco, Jesse Subject: RE: Questions for the MEX Phobos flyby Doy062-2010 preparation >For MEX tracking data we sample 1/60, however, we have the option to sample at 1/10 and 1/1. Aren't the TRK-2-34 data collected at 10/1 and it's during conversion to ODF that RMDC selects 1/60, 1/10, and 1/1? So ALL rates are always available in post-pass processing so long as the TRK-2-34 has not been lost. From susan.c.kurtik@jpl.nasa.gov Thu Feb 25 08:33:25 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion2.jpl.nasa.gov [128.149.139.106]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o1PGXMj01712 for ; Thu, 25 Feb 2010 08:33:22 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o1PGX1do007918 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Thu, 25 Feb 2010 08:33:03 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Thu, 25 Feb 2010 08:33:01 -0800 From: "Kurtik, Susan C (9020)" To: "mexmps@esa.int" CC: "Kern, Albert (9200-Affiliate)" , "Arroyo, Belinda (314E)" , "Kahan, Daniel S (332K)" , !DL-DSN-MPSETD , "Han, Don (343J)" , "Goltz, Gene L (332K)" , "Bell, Julia L (9020)" , "Bracamonte, Larry H" , "Stoloff, Michael J (316E)" , "Michel.Denis@esa.int" , mimsched , "Reboud, Olivier (9210-Affiliate)" , "Simpson, Richard A (6520-Affiliate)" , "Espinueva, Ruben P (314E)" , "Asmar, Sami W (332K)" , "stefan.remus@sciops.esa.int" , "Thompson, Thomas W (3300)" , "Wolfgang.Hell@esa.int" , "Kurtik, Susan C (9020)" Date: Thu, 25 Feb 2010 08:32:02 -0800 Subject: Re: MEX-DSN Phobos Test 24 Feb (MEX Phobos flyby Doy062-2010 preparation) Thread-Topic: MEX-DSN Phobos Test 24 Feb (MEX Phobos flyby Doy062-2010 preparation) Thread-Index: Acq2JRlEarK/DTiZQ5O7Hzd6l4QHeQAEvXC4 Message-ID: In-Reply-To: Accept-Language: en-US Content-Language: en X-MS-Has-Attach: yes X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/mixed; boundary="_004_C7ABE6028D8EASusanCKurtikjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: susan.c.kurtik@jpl.nasa.gov X-AUTH: Authorized Content-Length: 1772901 Status: RO --_004_C7ABE6028D8EASusanCKurtikjplnasagov_ Content-Type: multipart/alternative; boundary="_000_C7ABE6028D8EASusanCKurtikjplnasagov_" --_000_C7ABE6028D8EASusanCKurtikjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable The operations timeline is excellent, thanks for the response on the BOT-AOS delays to be expected. Best of luck on an exciting closest flyby. I have updated the package with the additional information on the telemetry downlink and included the operations timeline. Best regards On 2/25/10 6:15 AM, "mexmps@esa.int" wrote: Dear Susan, Thanks for the feedback. I was in the control room during the first test and everything went down as expected. BOT and AOS TM also happened as expected. The offset between BOT and AOS TM is due to various delays in the system. Sorry I didn't point that out during last week's teleconference. A carrier should have been acquired earlier (and was, as far as I could see). Due to current power constraints (we are in an eclipse season), we have to fully switch off the TX for as long as we are not transmitting. There are numerous wait times adding up before we see TM. These include a penalty wait after eclipse exit and a numbuer of wait times that the TX system needs to go from full-off to TM ON. For the Phobos flyby, I had to violate some of our eclipse operations rules to squeeze in the experiment. We leave the TX on for about twice as long as the currently allowed maximum for routine operations. It has to go to full- off during the eclipse (there is no way around that) but I switch it on right after eclipse exit (just an hour before CA) and configure it directly for coherent ranging. After running a couple of power analyses I decided to shave off some minutes, even if it means waiting a little after the BOT, to make extra sure our bat doesn't deplete below allowable limits (a safe mode would spoil our day I guess). As promised, I attach the annotated time line for the fly-by. If you have any questions, just ask. Cheers, Hannes. ... From rsimpson Thu Feb 25 16:39:36 2010 Return-Path: Received: (from rsimpson@localhost) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) id o1Q0dZm03244; Thu, 25 Feb 2010 16:39:35 -0800 (PST) Date: Thu, 25 Feb 2010 16:39:35 -0800 (PST) From: Dick Simpson 650-723-3525 Message-ID: <3243.1267144776@magellan> Mime-Version: 1.0 To: daniel.s.kahan@jpl.nasa.gov, rsimpson Subject: ODFs from DSN Phobos Tests Content-Type: multipart/mixed; boundary="-" Content-Length: 374657 Status: RO This is a MIME encoded message. Decode it with "munpack" or any other MIME reading software. Mpack/munpack is available via anonymous FTP in ftp.andrew.cmu.edu:pub/mpack/ --- Danny: This is what I sent to Europe; I have renamed the attached file odf.zap so it will get through the JPL censors. Just change the name to odf.zip and unzip it to get 10 ODFs covering days 051-056. Dick - - - - - - - - - - - - - - - - - - - - Martin, Tom, Pascal: The attached zip file contains all of the MEX ODFs from Phobos tests at DSN stations that have been released so far. You may find them useful for software exercises. The '1s' files are probably limited to the tests; the other files are 60-s data and may include other passes. These will be included in later 'monthly' deliveries; I thought you might like to have them available now even though they don't have the usual file names and PDS labels. Regards, Dick --- Content-Type: application/octet-stream; name="odf.zap" Content-Transfer-Encoding: base64 Content-Disposition: inline; filename="odf.zap" Content-MD5: tjXONM1RtXNnnRR54tOtyw== UEsDBBQAAAAIAM0DWjx7v/pINxMAAAA/AAAPABUAMTAwNTFPMDUzLlNDMDQxVVQJAAMhFodL IRaHS1V4BAAcBCkA7dt5OJX5+wfwc+zJsUT25Sj7ErJTskQJLdJUUymVrzaFaSNC2ddEUtla ... From daniel.s.kahan@jpl.nasa.gov Thu Feb 25 16:43:20 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion1.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o1Q0hKj03254 for ; Thu, 25 Feb 2010 16:43:20 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o1Q0hLpU018356 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL) for ; Thu, 25 Feb 2010 16:43:22 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Thu, 25 Feb 2010 16:43:21 -0800 From: "Kahan, Daniel S (332K)" To: "Simpson, Richard A (6520-Affiliate)" Date: Thu, 25 Feb 2010 16:43:20 -0800 Subject: RE: ODFs from DSN Phobos Tests Thread-Topic: ODFs from DSN Phobos Tests Thread-Index: Acq2fC87PZoaDuboRse5S5kxnUoURgAAGbog Message-ID: <79D001DEDB0DEC47A247B110F3E86682072E760220@ALTPHYEMBEVSP30.RES.AD.JPL> References: <3243.1267144776@magellan> In-Reply-To: <3243.1267144776@magellan> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: text/plain; charset="us-ascii" MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: daniel.s.kahan@jpl.nasa.gov X-AUTH: Authorized Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by magellan.stanford.edu id o1Q0hKj03254 Content-Length: 1129 Status: RO Thanks. For the actual flyby, Martin requested that we get the files to him ASAP. I will inquire of RMDC how fast they can do it for RSSG. -----Original Message----- From: Dick Simpson 650-723-3525 [mailto:rsimpson@magellan.stanford.edu] Sent: Thursday, February 25, 2010 4:40 PM To: Kahan, Daniel S (332K); Simpson, Richard A (6520-Affiliate) Subject: ODFs from DSN Phobos Tests Danny: This is what I sent to Europe; I have renamed the attached file odf.zap so it will get through the JPL censors. Just change the name to odf.zip and unzip it to get 10 ODFs covering days 051-056. Dick - - - - - - - - - - - - - - - - - - - - Martin, Tom, Pascal: The attached zip file contains all of the MEX ODFs from Phobos tests at DSN stations that have been released so far. You may find them useful for software exercises. The '1s' files are probably limited to the tests; the other files are 60-s data and may include other passes. These will be included in later 'monthly' deliveries; I thought you might like to have them available now even though they don't have the usual file names and PDS labels. Regards, Dick From daniel.s.kahan@jpl.nasa.gov Fri Feb 26 11:04:59 2010 Return-Path: Received: from mail.jpl.nasa.gov (smtp.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o1QJ4xj04927 for ; Fri, 26 Feb 2010 11:04:59 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap02.jpl.nasa.gov [128.149.137.73]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o1QJ4wNC021152 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL) for ; Fri, 26 Feb 2010 11:04:58 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP02.RES.AD.JPL ([128.149.137.73]) with mapi; Fri, 26 Feb 2010 11:04:58 -0800 From: "Kahan, Daniel S (332K)" To: "Simpson, Richard A (6520-Affiliate)" Date: Fri, 26 Feb 2010 11:04:57 -0800 Subject: RE: ODFs from DSN Phobos Tests Thread-Topic: ODFs from DSN Phobos Tests Thread-Index: Acq2ijJfPVUfvGI9TeKnnE9b5Qh9fAAi21ym Message-ID: <79D001DEDB0DEC47A247B110F3E86682072E3B4F99@ALTPHYEMBEVSP30.RES.AD.JPL> References: <201002260219.o1Q2Js703366@magellan.stanford.edu> In-Reply-To: <201002260219.o1Q2Js703366@magellan.stanford.edu> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: text/plain; charset="us-ascii" MIME-Version: 1.0 X-Source-IP: altvirehtstap02.jpl.nasa.gov [128.149.137.73] X-Source-Sender: daniel.s.kahan@jpl.nasa.gov X-AUTH: Authorized Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by magellan.stanford.edu id o1QJ4xj04927 Content-Length: 1004 Status: RO Looking over Martin's email exchange, mostly with Sami, I think he probably figures it can get to him the fastest coming straight from JPL, just like the processed data from the RSR will. I guess it is implied that we will get him the files, which is fine since Gene and/or I will already be covering the pass on the RSR. ________________________________________ From: Dick Simpson 650-723-3525 [rsimpson@magellan.stanford.edu] Sent: Thursday, February 25, 2010 6:19 PM To: Kahan, Daniel S (332K) Subject: RE: ODFs from DSN Phobos Tests >Thanks. For the actual flyby, Martin requested that we get the files >to him ASAP. I will inquire of RMDC how fast they can do it for RSSG. Does he want tyou to send him the files? I've heard nothing from him on this, and I'm (on paper) his data manager. My experience is that Wilson can turn these around in 24 hrs, maybe less. The flyby itself is in the middle of the day PST, so Thursday for the DSS 63 data should be pretty easy I would think. From mars_ops-bounces@sciops.esa.int Tue Mar 2 02:09:44 2010 Return-Path: Received: from esa-sf1.esa.gmessaging.net (esa-sf3.esa.gmessaging.net [194.51.201.69]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o22A9gj26424 for ; Tue, 2 Mar 2010 02:09:43 -0800 (PST) Received: from esa-sf1.esa.gmessaging.net (localhost [127.0.0.1]) by localhost.esa.gmessaging.net (Postfix) with SMTP id B9B1C249B2F for ; Tue, 2 Mar 2010 11:09:37 +0100 (CET) Received: from sciops-mailgw.vilspa.esa.int (sciops-mailgw.vilspa.esa.int [193.147.152.105]) by esa-sf1.esa.gmessaging.net (Postfix) with ESMTP id 80AD4249AFB for ; Tue, 2 Mar 2010 11:09:37 +0100 (CET) Received: from sciwww01.esac.esa.int (sciwww01.esac.esa.int [193.147.152.112]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id 7DB7A11FAC8 for ; Tue, 2 Mar 2010 11:09:42 +0100 (CET) Received: from sciwww01.esac.esa.int (localhost.localdomain [127.0.0.1]) by sciwww01.esac.esa.int (8.13.1/8.13.1) with ESMTP id o22A9gJ2022829 for ; Tue, 2 Mar 2010 11:09:42 +0100 Received: from sciops-mailgw.vilspa.esa.int (sciops-mailgw.vilspa.esa.int [193.147.152.105]) by sciwww01.esac.esa.int (8.13.1/8.13.1) with ESMTP id o22A9e4t022770 for ; Tue, 2 Mar 2010 11:09:40 +0100 Received: by sciops-mailgw.vilspa.esa.int (Postfix) id ED42011FACD; Tue, 2 Mar 2010 11:09:39 +0100 (CET) Delivered-To: mars_ops@sciops.esa.int Received: from sciwww01.esac.esa.int (sciwww01.esac.esa.int [193.147.152.112]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id C568D11FACC; Tue, 2 Mar 2010 11:09:39 +0100 (CET) Received: from sciwww01.esac.esa.int (localhost.localdomain [127.0.0.1]) by sciwww01.esac.esa.int (8.13.1/8.13.1) with ESMTP id o22A9dX2022727; Tue, 2 Mar 2010 11:09:39 +0100 Received: from sciops-mailgw.vilspa.esa.int (sciops-mailgw.vilspa.esa.int [193.147.152.105]) by sciwww01.esac.esa.int (8.13.1/8.13.1) with ESMTP id o22A9apZ022576 for ; Tue, 2 Mar 2010 11:09:36 +0100 Received: by sciops-mailgw.vilspa.esa.int (Postfix) id C9B8A11FACB; Tue, 2 Mar 2010 11:09:36 +0100 (CET) Delivered-To: mex_sciops@sciops.esa.int Received: from esacom94-int.estec.esa.int (esacom94-ext.estec.esa.int [131.176.107.3]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id 2C97811F8ED; Tue, 2 Mar 2010 11:09:36 +0100 (CET) Received: from esa-sf1.esa.gmessaging.net (esa-sf2.esa.gmessaging.net [194.51.201.68]) by esacom94-int.estec.esa.int (8.14.0/8.14.0/ESA-External-v4.0) with ESMTP id o22A9ZJY019968; Tue, 2 Mar 2010 10:09:35 GMT Received: from esa-sf1.esa.gmessaging.net (localhost [127.0.0.1]) by localhost.esa.gmessaging.net (Postfix) with SMTP id 376CE395B7E; Tue, 2 Mar 2010 11:09:30 +0100 (CET) Received: from rssd-gw.estec.esa.int (rssd-gw.estec.esa.int [195.169.141.1]) by esa-sf1.esa.gmessaging.net (Postfix) with ESMTP id 178D4395B7B; Tue, 2 Mar 2010 11:09:30 +0100 (CET) Received: from [127.0.0.1] ([131.176.13.67]) by rssd-gw.estec.esa.int (Sun Java System Messaging Server 6.2-7.05 (built Sep 5 2006)) with ESMTPSA id <0KYN00FD3G7YUT00@rssd-gw.estec.esa.int>; Tue, 02 Mar 2010 11:09:35 +0100 (CET) Date: Tue, 02 Mar 2010 11:08:40 +0100 From: "Fred A. Jansen" To: mexpi@sciops.esa.int, mex_sciops@sciops.esa.int, Mars Express Science Ground Segment Message-id: <15884_1267524577_4B8CE3E1_15884_197557_1_4B8CE3A8.80500@rssd.esa.int> MIME-version: 1.0 Content-type: text/plain; charset=ISO-8859-1; format=flowed Content-transfer-encoding: 7BIT User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.9.1.7) Gecko/20100111 Thunderbird/3.0.1 X-PMX-Version: 5.5.7.378829, Antispam-Engine: 2.7.2.376379, Antispam-Data: 2010.3.2.95720 X-BeenThere: mex_sciops@sciops.esa.int X-Mailman-Version: 2.1.5 Precedence: list Cc: Subject: [Mars_ops] [Mex_sciops] Phobos fly-by status X-BeenThere: mars_ops@sciops.esa.int List-Id: mars_ops.sciops.esa.int List-Unsubscribe: , List-Archive: List-Post: List-Help: List-Subscribe: , Sender: mars_ops-bounces@sciops.esa.int Errors-To: mars_ops-bounces@sciops.esa.int Content-Length: 3370 Status: R Dear Colleagues, A WWW story on the Phobos fly-by's has just been published at : http://www.esa.int/esaCP/SEMFKA6K56G_index_0.html In there you will see mention of an over performance of a recent OCM. I would like to briefly inform you about what happened. The 21-Feb-2010 OCM showed an overperformance of 0.68% (+11.6 mm/s). The 1-sigma uncertainty on this result is <0.01% (<0.1 mm/s). The apoapsis altitude was increased by 360 m more than planned and the period increased by 0.75 seconds more than planned. This over performance, while within the normal statistical margins, led to a (delta-)orbit change compared to what was predicted, and last Thu PM i received an advance warning that the latest FDyn predicts went in the direction of predicting an occultation of MEX by Phobos at closest flyby time. Apart from that, the actual orbit would be 10 km higher. At that time there was little that could be done, however FDyn soon came up with an alternative proposal. This consisted of a change in the WOLs this week, leading to no occultation on DOY 0062 by Phobos during the MEX close fly-by. This new WOL strategy however, will increase the phase error (from about 20 to about 30 seconds) to avoid to have the radio path occulted by Phobos. This strategy is easier to do than a manoeuvre on the short time period remaining before the flyby, and less costly than trying to avoid Phobos by reducing the phase error. The price to pay is : - a slightly higher distance at closest approach (77 km from Phobos center), but at least it is not interrupted ! - a temporary increased phase error. So, following the flyby on 3 March, a small correction manoeuvre (estimated ~ 13 cm/s) on 4 March will revert the phase error drift such that the following Phobos observation by HRSC (7 March) has a phase error similar or smaller to what it would be (~20 seconds) if we would do nothing than regular WOLs, and bring us back to zero phase error a few days later. Analysis shows that the radius (of the longest semi-axis) of Phobos would have to be artificially increased by at least 8 km to cause an occultation. The prediction is still for a very short eclipse of 3 seconds duration between 20:55:46 and 20:55:49 UTC. The prediction for the time of closest approach is 20:55:40 UTC with a miss distance from the centre of Phobos of 77 km. I hope to have sufficiently informed you, Kind Regards, Fred Jansen _______________________________________________ Mex_sciops mailing list Mex_sciops@sciops.esa.int http://www.sciops.esa.int/mailman/listinfo/mex_sciops _______________________________________________ Mars_ops mailing list Mars_ops@sciops.esa.int http://www.sciops.esa.int/mailman/listinfo/mars_ops From Thomas.W.Thompson@jpl.nasa.gov Wed Mar 3 00:46:51 2010 Return-Path: Received: from mail.jpl.nasa.gov (smtp.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o238kpj11126 for ; Wed, 3 Mar 2010 00:46:51 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o238kMLc002740 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Wed, 3 Mar 2010 00:46:23 -0800 Received: from ALTPHYEMBEVSP10.RES.AD.JPL ([172.16.0.11]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Wed, 3 Mar 2010 00:46:22 -0800 From: "Thompson, Thomas W (3300)" Date: Wed, 3 Mar 2010 00:46:26 -0800 Subject: Mars News - Mars Express heading for closest flyby of Phobos Thread-Topic: Mars News - Mars Express heading for closest flyby of Phobos Thread-Index: Acq6rgJZ3449C+bErE2UFGgEJ3/VXg== Message-ID: Accept-Language: en-US Content-Language: en X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/alternative; boundary="_000_C7B361E2E55BThomasWThompsonjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: Thomas.W.Thompson@jpl.nasa.gov X-AUTH: Authorized Content-Length: 9370 Status: RO --_000_C7B361E2E55BThomasWThompsonjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable http://www.esa.int/esaCP/SEMFKA6K56G_index_0.html Mars Express heading for closest flyby of Phobos European Space Agency 1 March 2010 ESA's Mars Express will skim the surface of Mars' largest moon Phobos on Wednesday evening. Passing by at an altitude of 67 km, precise radio tracking will allow researchers to peer inside the mysterious moon. Mars Express is currently engaged in a series of 12 flybys of Phobos. At each close pass, different instruments are trained towards the mysterious space rock, gaining new information. The closest flyby will take place on 3 March at 21:55 CET (20:55 GMT). From close range, Mars Express will be pulled 'off-course' by the gravitational field of Phobos. This will amount to no more than a few millimetres every second and will not affect the mission in any way. However, to the tracking teams on Earth, it will allow a unique look inside the moon to see how its mass is distributed throughout. How will the ground teams make these tremendously sensitive measurements? Ironically, they will turn off all data signals from the spacecraft. The only thing that the ground stations will listen out for is the 'carrier signal' -- the pure radio signal that is normally modulated to carry data. With no data on the carrier signal, the only thing that can modulate the signal is any change in its frequency caused by Phobos tugging the spacecraft. The changes will amount to variations of just one part in a trillion, and are a manifestation of the Doppler effect -- the same effect that causes an ambulance siren to change pitch as it zooms past. Two dress rehearsals for this exacting operation have already taken place, allowing ground station personnel and spacecraft controllers to practise their various roles. Now it is time to do it for real. Originally planned for 50 km altitude, Mars Express will now pass Phobos at 67 km. A slight 'over performance' during a manoeuvre last week had put the spacecraft on a trajectory that included an occultation by Phobos. This meant that Mars Express would pass behind Phobos as seen from Earth. As this would jeopardise the tracking measurements, it was decided to perform another manoeuvre to position the flyby at a slightly higher altitude than originally planned. After the closest flyby, the work is not over. Mars Express will sweep past Phobos a further seven times before the campaign is complete. In addition to the tracking experiment, known as MaRS for Mars Radio Science, the MARSIS radar has already been probing the subsurface of Phobos with radar beams. "We have performed a preliminary processing of the data and the Phobos signature is evident in almost all the data set," says Andrea Cicchetti, Italian Institute of Physics of Interplanetary Space, Rome, and one of the MARSIS team. The camera, HRSC, will be used on the 7 March flyby, when Mars Express passes over the daylight side of Phobos at an altitude of 107 km, and will continue to be used during all the subsequent flybys, obtaining high-resolution images of the moon's surface. The other instruments will also get their chance to work. ASPERA is already studying the way charged particles from the Sun interact with the surface of Phobos. SPICAM, PFS, OMEGA are characterising the surface of the moon, with PFS also aiming to measure the temperature of Phobos' day and night sides. HRSC will pay particular attention to the proposed landing site for the Russian Phobos-Grunt mission, which is expected to launch in 2011/12. "All the experiments on Mars Express have something to say about Phobos," says Olivier Witasse, Mars Express Project Scientist, ESA. This is a bonus for science, considering that none of them were originally designed to study Phobos the moon, only Mars the planet. The science results from these flybys are expected in subsequent weeks or months, when the various teams have had time to analyse the data. More information: Updates as the flybys take place will be posted on the Mars Express blog, http://webservices.esa.int/blog/blog/7 From wilson.chen@dsn.nasa.gov Wed Mar 3 10:14:23 2010 Return-Path: Received: from DSNOAM-MM.jpl.nasa.gov (dsnoam-mm.jpl.nasa.gov [128.149.207.83]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23IELj11995 for ; Wed, 3 Mar 2010 10:14:21 -0800 (PST) Received: from dsnoamex1.jpl.nasa.gov (Not Verified[128.149.207.88]) by DSNOAM-MM.jpl.nasa.gov with MailMarshal (v6,7,2,8378) id ; Wed, 03 Mar 2010 10:14:59 -0800 X-MimeOLE: Produced By Microsoft Exchange V6.5 Content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01CABAFD.590BF47D" Subject: 41 RMDC Radio Science Delivery Date: Wed, 3 Mar 2010 10:14:20 -0800 Message-ID: X-MS-Has-Attach: X-MS-TNEF-Correlator: Thread-Topic: 41 RMDC Radio Science Delivery Thread-Index: AcoMpLwnrYVmBHKJRlGFcNvJk8Md9ACM2+0gAMn6QCABPE/UIADtPmwgAY88RiAAPLpgIADCFpkgAgKgSyABUk9qIADKO0YgAJV+dCAAyZUkIACXzZAgAMjmliAAlnc8IAEpvWMgAZUNMSAA/FRsgANZkSbwFZk3A8AAPvo8EAElYx/g References: To: Cc: "!DL-DSN-RMDC" Content-Length: 4667 Status: RO This is a multi-part message in MIME format. ------_=_NextPart_001_01CABAFD.590BF47D Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: quoted-printable The listed files have been processed and delivered to: OSCARX://ftp/ras/sc41/odfs/10062O062_43X_1s.SC041 OSCARX://ftp/ras/sc41/odfs/10062O062_43S_1s.SC041 OSCARX://ftp/ras/sc41/odfs/10062O062_15X_1s.SC041 OSCARX://ftp/ras/sc41/odfs/10062O062_15S_1s.SC041 Regards, Wilson Chen RMDC Analyst Phone: 626-305-6269 Email: wcchen@jftl.jpl.nasa.gov wilson.chen@dsn.nasa.gov From mpaetzol@uni-koeln.de Wed Mar 3 13:11:09 2010 Return-Path: Received: from smtp-out.rrz.uni-koeln.de (smtp-out.rrz.uni-koeln.de [134.95.19.53]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23LB8j13734 for ; Wed, 3 Mar 2010 13:11:08 -0800 (PST) X-Virus-Scanned: amavisd-new at uni-koeln.de Received: from localhost (lvr12.rrz.uni-koeln.de [134.95.19.63]) by smtp-out.rrz.uni-koeln.de (8.13.8/8.13.8) with ESMTP id o23LARNs015560; Wed, 3 Mar 2010 22:10:28 +0100 Received: from p4FD894B8.dip0.t-ipconnect.de (p4FD894B8.dip0.t-ipconnect.de [79.216.148.184]) by webmail.uni-koeln.de (IMP) with HTTP for ; Wed, 03 Mar 2010 22:10:27 +0100 Message-ID: <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> Date: Wed, 03 Mar 2010 22:10:27 +0100 From: mpaetzol@uni-koeln.de To: mpaetzol@uni-koeln.de Cc: Bernd =?iso-8859-1?b?SOR1c2xlcg==?= , "werner.eidel@unibw-muenchen.de" , Tom Andert , "hannes.griebel@unibw-muenchen.de" , "riccardo.mattei@unibw-muenchen.de" , "martin.paetzold@uni-koeln.de" , Silvia Tellmann , "matthias.hahn@uni-koeln.de" , "thomas.kuerten@uni-koeln.de" , Janus , "kerstin.peter@uni-koeln.de" , Rokhsaneh boroumand , Ludmila Carone , "sascha.grziwa@uni-koeln.de" , "schoels@uni-koeln.de" , "Asmar, Sami W" , Daniel.S.Kahan@jpl.nasa.gov, Gene Goltz , Dehant Veronique , Pascal Rosenblatt , Ozgur Karatekin , len tyler , Dick Simpson 650-723-3525 , "Hinson, David P (6700-Affiliate)" , Paul Withers , Michael Mendillo , Michel Denis , Augustin Chicarro , Olivier Witasse , "Titov Dr., Dimitri" , Hakan Svedhem , tommy thompson , dwight.holmes@jpl.nasa.gov Subject: Re: Next joined MaRS/VeRa team meeting in Bonn: 18th and 19th March References: <4B8E68D9.3080903@uni-koeln.de> <1267647007.4b8ec21fcf43e@webmail.uni-koeln.de> <1267649063.4b8eca275fd45@webmail.uni-koeln.de> In-Reply-To: <1267649063.4b8eca275fd45@webmail.uni-koeln.de> MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: Internet Messaging Program (IMP) 3.2.6 X-Originating-IP: 79.216.148.184 X-Scanned-By: MIMEDefang 2.67 on 134.95.19.53 Content-Length: 1708 Status: RO We are through closest approach plus one light time and there was no occultation and MEX is still transmitting! Success!! :-) M. Zitat von mpaetzol@uni-koeln.de: > > Gene Goltz just told me that everything looks good at DSS63! > > Thanks, Gene! > M. > > > > > Zitat von mpaetzol@uni-koeln.de: > > > > > Dear Martians, > > > > I am at ESOC in the control room. It is 20:05 UT and Cebreros has just > > received X-band and S-band downlink from MEX. > > > > Presumably, DSS63 has too and that means we just started an experiment!!! > > > > Still less than one hour to closest approach at 20:55 UT. > > > > Keep your fingers crossed! > > > > Martin From owitasse@rssd.esa.int Wed Mar 3 13:17:31 2010 Return-Path: Received: from rssd-gw.estec.esa.int (rssd-gw.estec.esa.int [195.169.141.1]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23LHUj13774 for ; Wed, 3 Mar 2010 13:17:30 -0800 (PST) Received: from rssd.esa.int ([127.0.0.1]) by rssd-gw.estec.esa.int (Sun Java System Messaging Server 6.2-7.05 (built Sep 5 2006)) with ESMTP id <0KYQ00HTX5T59S60@rssd-gw.estec.esa.int> for rsimpson@magellan.stanford.edu; Wed, 03 Mar 2010 22:17:29 +0100 (CET) Received: from [82.237.200.147] by rssd-gw.estec.esa.int (mshttpd); Wed, 03 Mar 2010 22:17:29 +0100 Date: Wed, 03 Mar 2010 22:17:29 +0100 From: owitasse@rssd.esa.int Subject: Re: Next joined MaRS/VeRa team meeting in Bonn: 18th and 19th March In-reply-to: <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> To: mpaetzol@uni-koeln.de Cc: =?iso-8859-1?Q?Bernd_H=E4usler?= , "werner.eidel@unibw-muenchen.de" , Tom Andert , "hannes.griebel@unibw-muenchen.de" , "riccardo.mattei@unibw-muenchen.de" , "martin.paetzold@uni-koeln.de" , Silvia Tellmann , "matthias.hahn@uni-koeln.de" , "thomas.kuerten@uni-koeln.de" , Janus , "kerstin.peter@uni-koeln.de" , Rokhsaneh boroumand , Ludmila Carone , "sascha.grziwa@uni-koeln.de" , "schoels@uni-koeln.de" , "Asmar, Sami W" , Daniel.S.Kahan@jpl.nasa.gov, Gene Goltz , Dehant Veronique , Pascal Rosenblatt , Ozgur Karatekin , len tyler , Dick Simpson 650-723-3525 , "Hinson, David P (6700-Affiliate)" , Paul Withers , Michael Mendillo , Michel Denis , Augustin Chicarro , "Titov Dr., Dimitri" , Hakan Svedhem , tommy thompson , dwight.holmes@jpl.nasa.gov Message-id: MIME-version: 1.0 X-Mailer: Sun Java(tm) System Messenger Express 6.2-7.05 (built Sep 5 2006) Content-type: text/plain; charset=iso-8859-1 Content-language: en Content-disposition: inline X-Accept-Language: en Priority: normal References: <4B8E68D9.3080903@uni-koeln.de> <1267647007.4b8ec21fcf43e@webmail.uni-koeln.de> <1267649063.4b8eca275fd45@webmail.uni-koeln.de> <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by magellan.stanford.edu id o23LHUj13774 Content-Length: 2052 Status: R Great News! I look forward to seeing the results of the data analysis, and to learn more about the mysterious Phobos. Olivier From mpaetzol@uni-koeln.de Wed Mar 3 13:25:26 2010 Return-Path: Received: from smtp-out.rrz.uni-koeln.de (smtp-out.rrz.uni-koeln.de [134.95.19.53]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23LPQj13928 for ; Wed, 3 Mar 2010 13:25:26 -0800 (PST) X-Virus-Scanned: amavisd-new at uni-koeln.de Received: from localhost (lvr12.rrz.uni-koeln.de [134.95.19.63]) by smtp-out.rrz.uni-koeln.de (8.13.8/8.13.8) with ESMTP id o23LPOkP011614 for ; Wed, 3 Mar 2010 22:25:24 +0100 Received: from p4FD894B8.dip0.t-ipconnect.de (p4FD894B8.dip0.t-ipconnect.de [79.216.148.184]) by webmail.uni-koeln.de (IMP) with HTTP for ; Wed, 03 Mar 2010 22:25:24 +0100 Message-ID: <1267651524.4b8ed3c47c632@webmail.uni-koeln.de> Date: Wed, 03 Mar 2010 22:25:24 +0100 From: mpaetzol@uni-koeln.de To: Dick Simpson 650-723-3525 Subject: Re: Next joined MaRS/VeRa team meeting in Bonn: 18th and 19th March References: <201003032116.o23LGki13760@magellan.stanford.edu> In-Reply-To: <201003032116.o23LGki13760@magellan.stanford.edu> MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: Internet Messaging Program (IMP) 3.2.6 X-Originating-IP: 79.216.148.184 X-Scanned-By: MIMEDefang 2.67 on 134.95.19.53 Content-Length: 468 Status: R Dick, thank you! I wanted to ask you for that but I forgot! I was a nervous wreck today... :-) Zitat von Dick Simpson 650-723-3525 : > > >We are through closest approach plus one light time and there was no > occultation > >and MEX is still transmitting! > > The best news is that it's still transmitting. > > The pass ends in about 3 hours. If the data are > ready before I leave today, I will send them > via e-mail. > From sami.w.asmar@jpl.nasa.gov Wed Mar 3 13:31:07 2010 Return-Path: Received: from mail.jpl.nasa.gov (smtp.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23LV7j13962 for ; Wed, 3 Mar 2010 13:31:07 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o23LV5g8025855 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Wed, 3 Mar 2010 13:31:06 -0800 Received: from ALTPHYEMBEVSP20.RES.AD.JPL ([172.16.0.21]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Wed, 3 Mar 2010 13:31:04 -0800 Content-Type: multipart/mixed; boundary="_000_C7B415168A76samiwasmarjplnasagov_" From: "Asmar, Sami W (332K)" To: "mpaetzol@uni-koeln.de" CC: =?iso-8859-1?Q?Bernd_H=E4usler?= , "werner.eidel@unibw-muenchen.de" , Tom Andert , "hannes.griebel@unibw-muenchen.de" , "riccardo.mattei@unibw-muenchen.de" , "martin.paetzold@uni-koeln.de" , Silvia Tellmann , "matthias.hahn@uni-koeln.de" , "thomas.kuerten@uni-koeln.de" , Janus , "kerstin.peter@uni-koeln.de" , Rokhsaneh boroumand , Ludmila Carone , "sascha.grziwa@uni-koeln.de" , "schoels@uni-koeln.de" , "Kahan, Daniel S (332K)" , "Goltz, Gene L (332K)" , Dehant Veronique , Pascal Rosenblatt , Ozgur Karatekin , len tyler , "Simpson, Richard A (6520-Affiliate)" , "Hinson, David P (6700-Affiliate)" , Paul Withers , Michael Mendillo , Michel Denis , Augustin Chicarro , Olivier Witasse , "Titov Dr., Dimitri" , Hakan Svedhem , "Thompson, Thomas W (3300)" , "Holmes, Dwight P (9020)" Date: Wed, 3 Mar 2010 13:31:02 -0800 Subject: Closest Approach!! Thread-Topic: Closest Approach!! Thread-Index: Acq7FgraPBTuePB3RzG/pzY5NBRzxwAAse5Z Message-ID: In-Reply-To: <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: user-agent: Microsoft-Entourage/13.3.0.091002 acceptlanguage: en-US MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: sami.w.asmar@jpl.nasa.gov X-AUTH: Authorized Content-Length: 7351 Status: R --_000_C7B415168A76samiwasmarjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable Congratulations. From mpaetzol@uni-koeln.de Wed Mar 3 13:48:30 2010 Return-Path: Received: from smtp-out.rrz.uni-koeln.de (smtp-out.rrz.uni-koeln.de [134.95.19.53]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23LmTj13996 for ; Wed, 3 Mar 2010 13:48:29 -0800 (PST) X-Virus-Scanned: amavisd-new at uni-koeln.de Received: from localhost (lvr12.rrz.uni-koeln.de [134.95.19.63]) by smtp-out.rrz.uni-koeln.de (8.13.8/8.13.8) with ESMTP id o23Llmfx016830; Wed, 3 Mar 2010 22:47:48 +0100 Received: from p4FD894B8.dip0.t-ipconnect.de (p4FD894B8.dip0.t-ipconnect.de [79.216.148.184]) by webmail.uni-koeln.de (IMP) with HTTP for ; Wed, 03 Mar 2010 22:47:48 +0100 Message-ID: <1267652868.4b8ed90418fd5@webmail.uni-koeln.de> Date: Wed, 03 Mar 2010 22:47:48 +0100 From: mpaetzol@uni-koeln.de To: "Asmar, Sami W (332K)" Cc: Bernd =?iso-8859-1?b?SOR1c2xlcg==?= , "werner.eidel@unibw-muenchen.de" , Tom Andert , "hannes.griebel@unibw-muenchen.de" , "riccardo.mattei@unibw-muenchen.de" , "martin.paetzold@uni-koeln.de" , Silvia Tellmann , "matthias.hahn@uni-koeln.de" , "thomas.kuerten@uni-koeln.de" , Janus , "kerstin.peter@uni-koeln.de" , Rokhsaneh boroumand , Ludmila Carone , "sascha.grziwa@uni-koeln.de" , "schoels@uni-koeln.de" , "Kahan, Daniel S (332K)" , "Goltz, Gene L (332K)" , Dehant Veronique , Pascal Rosenblatt , Ozgur Karatekin , len tyler , "Simpson, Richard A (6520-Affiliate)" , "Hinson, David P (6700-Affiliate)" , Paul Withers , Michael Mendillo , Michel Denis , Augustin Chicarro , Olivier Witasse , "Titov Dr., Dimitri" , Hakan Svedhem , "Thompson, Thomas W (3300)" , "Holmes, Dwight P (9020)" Subject: Re: Closest Approach!! References: In-Reply-To: MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: Internet Messaging Program (IMP) 3.2.6 X-Originating-IP: 79.216.148.184 X-Scanned-By: MIMEDefang 2.67 on 134.95.19.53 Content-Length: 2162 Status: R Hi Sami, thanks for your support, guys! ESA is very excited here. Great job! Martin From dwight.p.holmes@jpl.nasa.gov Wed Mar 3 13:40:35 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion2.jpl.nasa.gov [128.149.139.106]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23LeYj13974 for ; Wed, 3 Mar 2010 13:40:34 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o23LeX1A007420 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Wed, 3 Mar 2010 13:40:33 -0800 Received: from ALTPHYEMBEVSP20.RES.AD.JPL ([172.16.0.21]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Wed, 3 Mar 2010 13:40:31 -0800 Content-Type: multipart/mixed; boundary="_000_B2C222C168B4004AB8E76917BE07CD11F00BDAAFDAALTPHYEMBEVSP_" From: "Holmes, Dwight P (9020)" To: "'mpaetzol@uni-koeln.de'" CC: =?iso-8859-1?Q?Bernd_H=E4usler?= , "werner.eidel@unibw-muenchen.de" , Tom Andert , "hannes.griebel@unibw-muenchen.de" , "riccardo.mattei@unibw-muenchen.de" , "martin.paetzold@uni-koeln.de" , Silvia Tellmann , "matthias.hahn@uni-koeln.de" , "thomas.kuerten@uni-koeln.de" , Janus , "kerstin.peter@uni-koeln.de" , Rokhsaneh boroumand , Ludmila Carone , "sascha.grziwa@uni-koeln.de" , "schoels@uni-koeln.de" , "Asmar, Sami W (332K)" , "Kahan, Daniel S (332K)" , "Goltz, Gene L (332K)" , Dehant Veronique , Pascal Rosenblatt , Ozgur Karatekin , len tyler , "Simpson, Richard A (6520-Affiliate)" , "Hinson, David P (6700-Affiliate)" , Paul Withers , Michael Mendillo , Michel Denis , Augustin Chicarro , Olivier Witasse , "Titov Dr., Dimitri" , Hakan Svedhem , "Thompson, Thomas W (3300)" Date: Wed, 3 Mar 2010 13:40:31 -0800 Subject: RE: Next joined MaRS/VeRa team meeting in Bonn: 18th and 19th March Thread-Topic: Next joined MaRS/VeRa team meeting in Bonn: 18th and 19th March Thread-Index: Acq7FgraPBTuePB3RzG/pzY5NBRzxwAA81eA Message-ID: References: <4B8E68D9.3080903@uni-koeln.de> <1267647007.4b8ec21fcf43e@webmail.uni-koeln.de> <1267649063.4b8eca275fd45@webmail.uni-koeln.de> <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> In-Reply-To: <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: dwight.p.holmes@jpl.nasa.gov X-AUTH: Authorized Content-Length: 11719 Status: RO --_000_B2C222C168B4004AB8E76917BE07CD11F00BDAAFDAALTPHYEMBEVSP_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable I would like to add my congratulations as well.=20 Regards, Dwight Holmes DSN Commitments Engineer Mars 2016 From sami.w.asmar@jpl.nasa.gov Wed Mar 3 13:55:35 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion2.jpl.nasa.gov [128.149.139.106]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23LtZj14035 for ; Wed, 3 Mar 2010 13:55:35 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap02.jpl.nasa.gov [128.149.137.73]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o23LtYDM019920 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Wed, 3 Mar 2010 13:55:34 -0800 Received: from ALTPHYEMBEVSP20.RES.AD.JPL ([172.16.0.21]) by ALTVIREHTSTAP02.RES.AD.JPL ([128.149.137.73]) with mapi; Wed, 3 Mar 2010 13:55:34 -0800 Content-Type: multipart/mixed; boundary="_000_C7B41AD28A88samiwasmarjplnasagov_" From: "Asmar, Sami W (332K)" To: "mpaetzol@uni-koeln.de" CC: =?iso-8859-1?Q?Bernd_H=E4usler?= , "werner.eidel@unibw-muenchen.de" , Tom Andert , "hannes.griebel@unibw-muenchen.de" , "riccardo.mattei@unibw-muenchen.de" , "martin.paetzold@uni-koeln.de" , Silvia Tellmann , "matthias.hahn@uni-koeln.de" , "thomas.kuerten@uni-koeln.de" , Janus , "kerstin.peter@uni-koeln.de" , Rokhsaneh boroumand , Ludmila Carone , "sascha.grziwa@uni-koeln.de" , "schoels@uni-koeln.de" , "Kahan, Daniel S (332K)" , "Goltz, Gene L (332K)" , Dehant Veronique , Pascal Rosenblatt , Ozgur Karatekin , len tyler , "Simpson, Richard A (6520-Affiliate)" , "Hinson, David P (6700-Affiliate)" , Paul Withers , Michael Mendillo , Michel Denis , Augustin Chicarro , Olivier Witasse , "Titov Dr., Dimitri" , Hakan Svedhem , "Thompson, Thomas W (3300)" , "Holmes, Dwight P (9020)" Date: Wed, 3 Mar 2010 13:55:30 -0800 Subject: Re: Closest Approach!! Thread-Topic: Closest Approach!! Thread-Index: Acq7G0Jsc6eENn2LTC2kXhGcgNrFsgAAPsks Message-ID: In-Reply-To: <1267652868.4b8ed90418fd5@webmail.uni-koeln.de> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: user-agent: Microsoft-Entourage/13.3.0.091002 acceptlanguage: en-US MIME-Version: 1.0 X-Source-IP: altvirehtstap02.jpl.nasa.gov [128.149.137.73] X-Source-Sender: sami.w.asmar@jpl.nasa.gov X-AUTH: Authorized Content-Length: 8160 Status: R --_000_C7B41AD28A88samiwasmarjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable We are excited too! From rsimpson Wed Mar 3 13:56:59 2010 Return-Path: Received: (from rsimpson@localhost) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) id o23LuxU14039; Wed, 3 Mar 2010 13:56:59 -0800 (PST) Date: Wed, 3 Mar 2010 13:56:59 -0800 (PST) From: Dick Simpson 650-723-3525 Message-Id: <201003032156.o23LuxU14039@magellan.stanford.edu> To: mpaetzol@uni-koeln.de, rsimpson Subject: Phobos Data Content-Length: 422 Status: RO > thank you! I wanted to ask you for that but I forgot! The MEX Data Manager is not a nervous wreck and will send the bits. I understand from RMDCT that they should have the DSS 63 ODF shortly after the pass ends. I have already received messages that the DSS 15 and DSS 43 data have been posted. The post- encounter DSS 14 data wilkl probably not be available until tomorrow morning (California time). From mpaetzol@uni-koeln.de Wed Mar 3 14:01:04 2010 Return-Path: Received: from smtp-out.rrz.uni-koeln.de (smtp-out.rrz.uni-koeln.de [134.95.19.53]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23M13j14069 for ; Wed, 3 Mar 2010 14:01:03 -0800 (PST) X-Virus-Scanned: amavisd-new at uni-koeln.de Received: from localhost (lvr12.rrz.uni-koeln.de [134.95.19.63]) by smtp-out.rrz.uni-koeln.de (8.13.8/8.13.8) with ESMTP id o23M0NI4006286; Wed, 3 Mar 2010 23:00:24 +0100 Received: from p4FD894B8.dip0.t-ipconnect.de (p4FD894B8.dip0.t-ipconnect.de [79.216.148.184]) by webmail.uni-koeln.de (IMP) with HTTP for ; Wed, 03 Mar 2010 23:00:23 +0100 Message-ID: <1267653623.4b8edbf7720ec@webmail.uni-koeln.de> Date: Wed, 03 Mar 2010 23:00:23 +0100 From: mpaetzol@uni-koeln.de To: mpaetzol@uni-koeln.de Cc: Bernd =?iso-8859-1?b?SOR1c2xlcg==?= , "werner.eidel@unibw-muenchen.de" , Tom Andert , "hannes.griebel@unibw-muenchen.de" , "riccardo.mattei@unibw-muenchen.de" , "martin.paetzold@uni-koeln.de" , Silvia Tellmann , "matthias.hahn@uni-koeln.de" , "thomas.kuerten@uni-koeln.de" , Janus , "kerstin.peter@uni-koeln.de" , Rokhsaneh boroumand , Ludmila Carone , "sascha.grziwa@uni-koeln.de" , "schoels@uni-koeln.de" , "Asmar, Sami W" , Daniel.S.Kahan@jpl.nasa.gov, Gene Goltz , Dehant Veronique , Pascal Rosenblatt , Ozgur Karatekin , len tyler , Dick Simpson 650-723-3525 , "Hinson, David P (6700-Affiliate)" , Paul Withers , Michael Mendillo , Michel Denis , Augustin Chicarro , Olivier Witasse , "Titov Dr., Dimitri" , Hakan Svedhem , tommy thompson , dwight.holmes@jpl.nasa.gov Subject: Re: Next joined MaRS/VeRa team meeting in Bonn: 18th and 19th March References: <4B8E68D9.3080903@uni-koeln.de> <1267647007.4b8ec21fcf43e@webmail.uni-koeln.de> <1267649063.4b8eca275fd45@webmail.uni-koeln.de> <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> In-Reply-To: <1267650627.4b8ed043a4a99@webmail.uni-koeln.de> MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: Internet Messaging Program (IMP) 3.2.6 X-Originating-IP: 79.216.148.184 X-Scanned-By: MIMEDefang 2.67 on 134.95.19.53 Content-Length: 2350 Status: R Friends, it is now 21:52 UT and Cebreros went off as back-up. Nothing to watch from ESOC any more. DSS63 will record the signal for another couple of hours. Everybody was very excited here. Lots of PR coverage. Many thanks to the MEX FCT, ESOC PR, DSS63, Cebreros, Sami, Danny, Gene. I feel relieved and will retire now... to the Australian bar having a beer... :-) Now, let's have fun with the data! Thanks and take care! Martin From mpaetzol@uni-koeln.de Wed Mar 3 14:01:56 2010 Return-Path: Received: from smtp-out.rrz.uni-koeln.de (smtp-out.rrz.uni-koeln.de [134.95.19.53]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23M1tj14073 for ; Wed, 3 Mar 2010 14:01:55 -0800 (PST) X-Virus-Scanned: amavisd-new at uni-koeln.de Received: from localhost (lvr12.rrz.uni-koeln.de [134.95.19.63]) by smtp-out.rrz.uni-koeln.de (8.13.8/8.13.8) with ESMTP id o23M1rg7011936 for ; Wed, 3 Mar 2010 23:01:54 +0100 Received: from p4FD894B8.dip0.t-ipconnect.de (p4FD894B8.dip0.t-ipconnect.de [79.216.148.184]) by webmail.uni-koeln.de (IMP) with HTTP for ; Wed, 03 Mar 2010 23:01:53 +0100 Message-ID: <1267653713.4b8edc51eb80c@webmail.uni-koeln.de> Date: Wed, 03 Mar 2010 23:01:53 +0100 From: mpaetzol@uni-koeln.de To: Dick Simpson 650-723-3525 Subject: Re: Phobos Data References: <201003032156.o23LuxU14039@magellan.stanford.edu> In-Reply-To: <201003032156.o23LuxU14039@magellan.stanford.edu> MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: Internet Messaging Program (IMP) 3.2.6 X-Originating-IP: 79.216.148.184 X-Scanned-By: MIMEDefang 2.67 on 134.95.19.53 Content-Length: 547 Status: R Dick, that's great!!! :-) Zitat von Dick Simpson 650-723-3525 : > > > thank you! I wanted to ask you for that but I forgot! > > The MEX Data Manager is not a nervous wreck and will > send the bits. I understand from RMDCT that they > should have the DSS 63 ODF shortly after the pass > ends. I have already received messages that the > DSS 15 and DSS 43 data have been posted. The post- > encounter DSS 14 data wilkl probably not be available > until tomorrow morning (California time). > From wilson.chen@dsn.nasa.gov Wed Mar 3 16:42:21 2010 Return-Path: Received: from DSNOAM-MM.jpl.nasa.gov (dsnoam-mm.jpl.nasa.gov [128.149.207.83]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o240gLj14495 for ; Wed, 3 Mar 2010 16:42:21 -0800 (PST) Received: from dsnoamex1.jpl.nasa.gov (Not Verified[128.149.207.88]) by DSNOAM-MM.jpl.nasa.gov with MailMarshal (v6,7,2,8378) id ; Wed, 03 Mar 2010 16:43:01 -0800 X-MimeOLE: Produced By Microsoft Exchange V6.5 Content-class: urn:content-classes:message MIME-Version: 1.0 Content-Type: multipart/alternative; boundary="----_=_NextPart_001_01CABB33.1A54815C" Subject: 41 RMDC Radio Science Delivery Date: Wed, 3 Mar 2010 16:39:08 -0800 Message-ID: X-MS-Has-Attach: X-MS-TNEF-Correlator: Thread-Topic: 41 RMDC Radio Science Delivery Thread-Index: AcoMpLwnrYVmBHKJRlGFcNvJk8Md9ACM2+0gAMn6QCABPE/UIADtPmwgAY88RiAAPLpgIADCFpkgAgKgSyABUk9qIADKO0YgAJV+dCAAyZUkIACXzZAgAMjmliAAlnc8IAEpvWMgAZUNMSAA/FRsgANZkSbwFZk3A8AAPvo8EAElYx/gAA1xqkA= References: To: Cc: "!DL-DSN-RMDC" Content-Length: 4444 Status: R This is a multi-part message in MIME format. ------_=_NextPart_001_01CABB33.1A54815C Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: quoted-printable The listed files have been processed and delivered to: OSCARX://ftp/ras/sc41/odfs/10062O062_63X_1s.SC041 OSCARX://ftp/ras/sc41/odfs/10062O062_63S_1s.SC041 Regards, Wilson Chen RMDC Analyst Phone: 626-305-6269 Email: wcchen@jftl.jpl.nasa.gov wilson.chen@dsn.nasa.gov From rsimpson Wed Mar 3 17:01:24 2010 Return-Path: Received: (from rsimpson@localhost) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) id o2411NH14552; Wed, 3 Mar 2010 17:01:23 -0800 (PST) Date: Wed, 3 Mar 2010 17:01:23 -0800 (PST) From: Dick Simpson 650-723-3525 Message-ID: <14551.1267664484@magellan> Mime-Version: 1.0 To: mpaetzol@uni-koeln.de, pascal.rosenblatt@oma.be, Tom.Andert@unibw.de, len.tyler@stanford.edu, rsimpson Subject: Phobos ODFs Content-Type: multipart/mixed; boundary="-" Content-Length: 967619 Status: R This is a MIME encoded message. Decode it with "munpack" or any other MIME reading software. Mpack/munpack is available via anonymous FTP in ftp.andrew.cmu.edu:pub/mpack/ --- Martin, Tom, Pascal, ... Attached is a zip file containing 1-second S- and X-Band ODFs from today's DSN tracking of MEX. Each pass is in a separate file, so there are files from DSS 15, 43, and 63. There are also two files with 60-s data, probably from multiple stations and both bands. There should be another pair of files tomorrow from the DSS 14 pass which begins in about three hours and ends at 0835. We expect to hear about profound new discoveries regarding Phobos shortly. Regards, Dick --- Content-Type: application/octet-stream; name="odf.zip" Content-Transfer-Encoding: base64 Content-Disposition: inline; filename="odf.zip" Content-MD5: TADvp6hoEz/qSeXbuF6Fuw== UEsDBBQAAAAIAIUGZDx8Re+JNL8AAIDUAgAVABUAMTAwNjIwNjJfNDNTXzFzLlNDMDQxVVQJ AAM6BI9LOgSPS1V4BAAcBCkAdNtpWM7pAsfx/rdoUdG+at9XpbRhJGVJSRKyZ98i20yMfctO ... From daniel.s.kahan@jpl.nasa.gov Wed Mar 3 14:32:05 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion1.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23MW5j14165 for ; Wed, 3 Mar 2010 14:32:05 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap02.jpl.nasa.gov [128.149.137.73]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o23MW6kK003264 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL) for ; Wed, 3 Mar 2010 14:32:06 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP02.RES.AD.JPL ([128.149.137.73]) with mapi; Wed, 3 Mar 2010 14:32:06 -0800 Content-Type: multipart/mixed; boundary="_000_79D001DEDB0DEC47A247B110F3E86682072E3B4FA3ALTPHYEMBEVSP_" From: "Kahan, Daniel S (332K)" To: "Simpson, Richard A (6520-Affiliate)" CC: "Asmar, Sami W (332K)" , "Goltz, Gene L (332K)" Date: Wed, 3 Mar 2010 14:28:02 -0800 Subject: MEX 2010-062 Gravity Field Data Thread-Topic: MEX 2010-062 Gravity Field Data Thread-Index: AQHKuyFaYIlzWlGf60i78erlV2MD7w== Message-ID: <79D001DEDB0DEC47A247B110F3E86682072E3B4FA3@ALTPHYEMBEVSP30.RES.AD.JPL> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: <79D001DEDB0DEC47A247B110F3E86682072E3B4FA3@ALTPHYEMBEVSP30.RES.AD.JPL> acceptlanguage: en-US MIME-Version: 1.0 X-Source-IP: altvirehtstap02.jpl.nasa.gov [128.149.137.73] X-Source-Sender: daniel.s.kahan@jpl.nasa.gov X-AUTH: Authorized Content-Length: 5008 Status: O --_000_79D001DEDB0DEC47A247B110F3E86682072E3B4FA3ALTPHYEMBEVSP_ Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: quoted-printable Dick, MEX Gravity Field Experiments on 2010-062 were conducted at DSS-15 and DSS-43. RSR open-loop data were recorded and played back to your MEX directory on rsops2 as follows: DSS-15 - X-band, 2-way - RSR2B1 - 2 kHz, 16 bits - 06:05:00 - 08:25:00 and: - S-band, 2-way - RSR2A1 - 2 kHz, 16 bits - 06:05:00 - 08:25:00 DSS-43 - X-band, 2-way - RSR2B1 - 2 kHz, 16 bits - 09:33:00 - 10:57:00 and: - S-band, 2-way - RSR2A1 - 2 kHz, 16 bits - 09:33:00 - 10:57:00 NOTES: 1) these recordings were done "in the blind" using scripts - Regards, Gene & Danny From daniel.s.kahan@jpl.nasa.gov Wed Mar 3 14:20:14 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion1.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23MKEj14152 for ; Wed, 3 Mar 2010 14:20:14 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o23MKDB5028369 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL) for ; Wed, 3 Mar 2010 14:20:13 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Wed, 3 Mar 2010 14:20:13 -0800 Content-Type: multipart/mixed; boundary="_000_79D001DEDB0DEC47A247B110F3E86682072E3B4FA2ALTPHYEMBEVSP_" From: "Kahan, Daniel S (332K)" To: "Simpson, Richard A (6520-Affiliate)" CC: "Asmar, Sami W (332K)" , "Goltz, Gene L (332K)" Date: Wed, 3 Mar 2010 14:16:40 -0800 Subject: MEX 2010-062 Gravity Field & Occultation Data Thread-Topic: MEX 2010-062 Gravity Field & Occultation Data Thread-Index: AQHKux+xzF7b/I9DBkuUZvDubWLp2w== Message-ID: <79D001DEDB0DEC47A247B110F3E86682072E3B4FA2@ALTPHYEMBEVSP30.RES.AD.JPL> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: <79D001DEDB0DEC47A247B110F3E86682072E3B4FA2@ALTPHYEMBEVSP30.RES.AD.JPL> acceptlanguage: en-US MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: daniel.s.kahan@jpl.nasa.gov X-AUTH: Authorized Content-Length: 4860 Status: O --_000_79D001DEDB0DEC47A247B110F3E86682072E3B4FA2ALTPHYEMBEVSP_ Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: quoted-printable Dick, A MEX Gravity Field Experiment and Occultation on 2010-062 were conducted at DSS-63. RSR open-loop data were recorded and played back to your MEX directory on rsops2 as follows: - X-band, 2-way - RSR2B1 - 2 kHz, 16 bits - 17:05:00 - 19:19:00 and: - S-band, 2-way - RSR2A1 - 2 kHz, 16 bits - 17:05:00 - 19:19:00 NOTES: 1) these recordings were performed in real time - Regards, Gene & Danny From gene.goltz@jpl.nasa.gov Wed Mar 3 16:25:06 2010 Return-Path: Received: from mail.jpl.nasa.gov (mailhost.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o240P5j14395 for ; Wed, 3 Mar 2010 16:25:05 -0800 (PST) Received: from ggoltz-xp.jpl.nasa.gov (ggoltz-2k.jpl.nasa.gov [137.78.78.47]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o240P5t5001191 (using TLSv1/SSLv3 with cipher DHE-RSA-AES256-SHA (256 bits) verified NO); Wed, 3 Mar 2010 16:25:06 -0800 Message-Id: <6.2.5.6.2.20100303161750.01ff7810@jpl.nasa.gov> X-Mailer: QUALCOMM Windows Eudora Version 6.2.5.6 Date: Wed, 03 Mar 2010 16:25:06 -0800 To: Dick Simpson 650-723-3525 From: Gene Goltz Subject: MEX 2009-062 Phobos Flyby Data Cc: Sami Asmar , Daniel.S.Kahan@jpl.nasa.gov Mime-Version: 1.0 Content-Type: text/plain; charset="us-ascii"; format=flowed X-Source-IP: ggoltz-2k.jpl.nasa.gov [137.78.78.47] X-Source-Sender: gene.goltz@jpl.nasa.gov X-AUTH: Authorized Content-Length: 485 Status: O Dick, A MEX flyby of Phobos was conducted at DSS-63 on 2010-062 (closest approach at about 21:02:15 UTC). RSR open-loop data were recorded and played back to your MEX directory on rsops2 as follows: - X-band, 2-way - RSR2B1 - 2 kHz, 16 bits - 20:16:00 to 23:47:00 and: - S-band, 2-way - RSR2A1 - 2 kHz, 16 bits - 20:16:00 to 23:47:00 NOTES: 1) these recordings were performed in real time - Regards, Gene & Danny From susan.c.kurtik@jpl.nasa.gov Wed Mar 3 15:01:31 2010 Return-Path: Received: from mail.jpl.nasa.gov (mailhost.jpl.nasa.gov [128.149.139.106]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23N1Uj14187 for ; Wed, 3 Mar 2010 15:01:30 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o23N1AX7029536 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Wed, 3 Mar 2010 15:01:11 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Wed, 3 Mar 2010 15:01:10 -0800 From: "Kurtik, Susan C (9020)" To: "Kurtik, Susan C (9020)" , "mexmps@esa.int" CC: "Kern, Albert (9200-Affiliate)" , "Arroyo, Belinda (314E)" , "Kahan, Daniel S (332K)" , !DL-DSN-MPSETD , "Han, Don (343J)" , "Goltz, Gene L (332K)" , "Bell, Julia L (9020)" , "Bracamonte, Larry H" , "Stoloff, Michael J (316E)" , "Michel.Denis@esa.int" , mimsched , "Reboud, Olivier (9210-Affiliate)" , "Simpson, Richard A (6520-Affiliate)" , "Espinueva, Ruben P (314E)" , "Asmar, Sami W (332K)" , "stefan.remus@sciops.esa.int" , "Thompson, Thomas W (3300)" , "Wolfgang.Hell@esa.int" Date: Wed, 3 Mar 2010 15:01:01 -0800 Subject: MEX-DSN Phobos Flyby Support Thread-Topic: MEX-DSN Phobos Flyby Support Thread-Index: Acq2JRlEarK/DTiZQ5O7Hzd6l4QHeQAEvXC4ATtVZ6Y= Message-ID: In-Reply-To: Accept-Language: en-US Content-Language: en X-MS-Has-Attach: yes X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/mixed; boundary="_005_C7B42A308DE36SusanCKurtikjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: susan.c.kurtik@jpl.nasa.gov X-AUTH: Authorized Content-Length: 311764 Status: RO --_005_C7B42A308DE36SusanCKurtikjplnasagov_ Content-Type: multipart/alternative; boundary="_000_C7B42A308DE36SusanCKurtikjplnasagov_" --_000_C7B42A308DE36SusanCKurtikjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable Congratulations to the MEX mission on your successful and exciting flyby of= Phobos! The NOPE reports that the DSN support of the Phobos flyby was nominal. DSS-= 63 remained 2-way throughout the flyby with S and X-band RCV in lock. Jesse From susan.c.kurtik@jpl.nasa.gov Wed Mar 3 15:03:31 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion1.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o23N3Vj14195 for ; Wed, 3 Mar 2010 15:03:31 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap02.jpl.nasa.gov [128.149.137.73]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o23N39fj021661 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Wed, 3 Mar 2010 15:03:10 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP02.RES.AD.JPL ([128.149.137.73]) with mapi; Wed, 3 Mar 2010 15:03:09 -0800 From: "Kurtik, Susan C (9020)" To: "Kurtik, Susan C (9020)" , "mexmps@esa.int" CC: "Kern, Albert (9200-Affiliate)" , "Arroyo, Belinda (314E)" , "Kahan, Daniel S (332K)" , !DL-DSN-MPSETD , "Han, Don (343J)" , "Goltz, Gene L (332K)" , "Bell, Julia L (9020)" , "Bracamonte, Larry H" , "Stoloff, Michael J (316E)" , "Michel.Denis@esa.int" , mimsched , "Reboud, Olivier (9210-Affiliate)" , "Simpson, Richard A (6520-Affiliate)" , "Espinueva, Ruben P (314E)" , "Asmar, Sami W (332K)" , "stefan.remus@sciops.esa.int" , "Thompson, Thomas W (3300)" , "Wolfgang.Hell@esa.int" Date: Wed, 3 Mar 2010 15:02:59 -0800 Subject: Re: MEX-DSN Phobos Flyby Support Thread-Topic: MEX-DSN Phobos Flyby Support Thread-Index: Acq2JRlEarK/DTiZQ5O7Hzd6l4QHeQAEvXC4ATtVZ6YAABGVUA== Message-ID: In-Reply-To: Accept-Language: en-US Content-Language: en X-MS-Has-Attach: yes X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/mixed; boundary="_005_C7B42AA68DE39SusanCKurtikjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap02.jpl.nasa.gov [128.149.137.73] X-Source-Sender: susan.c.kurtik@jpl.nasa.gov X-AUTH: Authorized Content-Length: 215697 Status: RO --_005_C7B42AA68DE39SusanCKurtikjplnasagov_ Content-Type: multipart/alternative; boundary="_000_C7B42AA68DE39SusanCKurtikjplnasagov_" --_000_C7B42AA68DE39SusanCKurtikjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable Jesse has generated a profile of DSS-63 uplink tune with a transmitter on t= ime of 164852 UTC. On 3/3/10 3:01 PM, "Kurtik, Susan C (9020)" w= rote: Congratulations to the MEX mission on your successful and exciting flyby of= Phobos! The NOPE reports that the DSN support of the Phobos flyby was nominal. DSS-= 63 remained 2-way throughout the flyby with S and X-band RCV in lock. Jesse -- Susan C. Kurtik Jet Propulsion Laboratory Deep Space Network Mission Support Manager 818 354-3598 office 818 687-7903 cell Don't leave earth without us From Michel.Denis@esa.int Thu Mar 4 08:05:52 2010 Return-Path: Received: from esacom90-int.esrin.esa.int (esacom90-ext.esrin.esa.int [192.171.5.18]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o24G5oj20815 for ; Thu, 4 Mar 2010 08:05:50 -0800 (PST) Received: from esacom66.esrin.esa.int (192-171-5-30.esrin.esa.int [192.171.5.30]) by esacom90-int.esrin.esa.int (8.13.3/8.13.3/ESA-External-v4.0) with ESMTP id o24G5l14019897; Thu, 4 Mar 2010 16:05:47 GMT Received: from esrinmta1.esrin.esa.int (esrinnotesadmin-a.esrin.esa.int [193.204.225.153]) by esacom66.esrin.esa.int (8.12.10/8.12.10/ESA-Internal-v3.2) with ESMTP id o24G5jbG025236; Thu, 4 Mar 2010 16:05:45 GMT In-Reply-To: Subject: MEX Phobos flyby 3 March 2010 --- Thanks! To: "Kurtik, Susan C (9020)" Cc: owitasse@rssd.esa.int, "Fred A. Jansen" , "Kern, Albert (9200-Affiliate)" , "Arroyo, Belinda (314E)" , "Kahan, Daniel S (332K)" , !DL-DSN-MPSETD , "Han, Don (343J)" , "Goltz, Gene L (332K)" , "Bell, Julia L (9020)" , "Bracamonte, Larry H" , "mexmps@esa.int" , "Stoloff, Michael J (316E)" , "Michel.Denis@esa.int" , mimsched , "Reboud, Olivier (9210-Affiliate)" , "Simpson, Richard A (6520-Affiliate)" , "Espinueva, Ruben P (314E)" , "Asmar, Sami W (332K)" , "stefan.remus@sciops.esa.int" , "Kurtik, Susan C (9020)" , "Thompson, Thomas W (3300)" , "Wolfgang.Hell@esa.int" X-Mailer: Lotus Notes Release 6.5.5 November 30, 2005 Message-ID: From: Michel.Denis@esa.int Date: Thu, 4 Mar 2010 17:05:44 +0100 X-MIMETrack: Serialize by Router on esrinmta1/esrin/ESA at 03/04/2010 17:05:46 MIME-Version: 1.0 Content-type: text/plain; charset=US-ASCII Content-Length: 701 Status: RO Dear DSN and JPL colleagues, Also on behalf of Olivier Witasse (MEX Project Scientist) and Fred Jansen (MEX Mission Manager), we would like to express our warm thanks and congratulations to all the personnel involved in the flawless preparation and execution of the Phobos flyby yesterday. We already heard that the data are of excellent quality and are looking forward to the science results! Kind regards, ---------------------------------------------------------------------------- Michel DENIS Head of the MARS EXPRESS Mission Operations Unit ESA / ESOC, Robert-Bosch-Str.5, 64293 DARMSTADT ---------------------------------------------------------------------------- From tom.andert@unibw.de Wed Mar 3 23:30:04 2010 Return-Path: Received: from gold2srv.rz.unibw-muenchen.de (gold2srv.RZ.UniBw-Muenchen.de [137.193.6.46]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o247U3j20172 for ; Wed, 3 Mar 2010 23:30:04 -0800 (PST) X-IronPort-Anti-Spam-Filtered: true X-IronPort-Anti-Spam-Result: As4EAEbwjkuJwU8S/2dsb2JhbACFZ78fCY1QgmuCEQSONw X-IronPort-AV: E=McAfee;i="5400,1158,5909"; a="3786240" X-IronPort-AV: E=Sophos;i="4.49,580,1262559600"; d="scan'208";a="3786240" Received: from maxus.lrt.unibw-muenchen.de (HELO [137.193.79.18]) ([137.193.79.18]) by gold2srv.rz.unibw-muenchen.de with ESMTP/TLS/DHE-RSA-CAMELLIA256-SHA; 04 Mar 2010 08:30:04 +0100 Message-ID: <4B8F6174.4050901@unibw.de> Date: Thu, 04 Mar 2010 08:29:56 +0100 From: Thomas Andert User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.2; de; rv:1.9.1.7) Gecko/20100111 Lightning/1.0b1 Thunderbird/3.0.1 MIME-Version: 1.0 To: rsimpson@magellan.stanford.edu Subject: Re: [POSSIBLE VIRUS:###] Phobos ODFs References: <17698_1267664487_4B8F0666_17698_2218_1_14551.1267664484@magellan> In-Reply-To: <17698_1267664487_4B8F0666_17698_2218_1_14551.1267664484@magellan> Content-Type: text/plain; charset=ISO-8859-15; format=flowed Content-Transfer-Encoding: 8bit Content-Length: 934 Status: RO Dear Dick, thanks a lot for the fast transfer of the data. best regards, Tom Am 04.03.2010 02:01, schrieb Dick Simpson 650-723-3525: > Martin, Tom, Pascal, ... > > Attached is a zip file containing 1-second S- and X-Band > ODFs from today's DSN tracking of MEX. Each pass is in a > separate file, so there are files from DSS 15, 43, and 63. > There are also two files with 60-s data, probably from > multiple stations and both bands. > > There should be another pair of files tomorrow from the > DSS 14 pass which begins in about three hours and ends at > 0835. > > We expect to hear about profound new discoveries regarding > Phobos shortly. > > Regards, > Dick > -- Tom Andert Institut fur Raumfahrttechnik LRT-9 Fakultat fur Luft-und Raumfahrttechnik Universitat der Bundeswehr Munchen Werner-Heisenberg-Weg 39 85577 Neubiberg Tel.: +49-89-6004-3598 Fax.: +49-89-6004-2138 E-Mail:tom.andert@unibw.de From mpaetzol@uni-koeln.de Thu Mar 4 05:04:08 2010 Return-Path: Received: from smtp-out.rrz.uni-koeln.de (smtp-out.rrz.uni-koeln.de [134.95.19.53]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o24D46j20676 for ; Thu, 4 Mar 2010 05:04:06 -0800 (PST) X-Virus-Scanned: amavisd-new at uni-koeln.de Received: from smtp.uni-koeln.de (milter4.rrz.uni-koeln.de [134.95.19.193]) by smtp-out.rrz.uni-koeln.de (8.13.8/8.13.8) with ESMTP id o24D452l023230; Thu, 4 Mar 2010 14:04:05 +0100 X-MSA-SIP: paris.planet.uni-koeln.de [134.95.38.5] Received: from [134.95.38.5] (paris.planet.uni-koeln.de [134.95.38.5]) by smtp.uni-koeln.de (8.13.8/8.13.8) with ESMTP id o24D444I026707; Thu, 4 Mar 2010 14:04:05 +0100 Message-ID: <4B8FAFF9.20304@uni-koeln.de> Date: Thu, 04 Mar 2010 14:04:57 +0100 From: =?ISO-8859-15?Q?Martin_P=E4tzold?= User-Agent: Thunderbird 2.0.0.23 (Windows/20090812) MIME-Version: 1.0 To: Dick Simpson 650-723-3525 CC: pascal.rosenblatt@oma.be, Tom.Andert@unibw.de, len.tyler@stanford.edu Subject: Re: [POSSIBLE VIRUS:###] Phobos ODFs References: <17698_1267664487_4B8F0666_17698_2218_1_14551.1267664484@magellan> In-Reply-To: <17698_1267664487_4B8F0666_17698_2218_1_14551.1267664484@magellan> Content-Type: text/plain; charset=ISO-8859-15; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.67 on 134.95.19.53 Content-Length: 760 Status: RO Hi Dick, I just returned to Cologne. Thanks for the data. Tom is already computing the predict based on a preliminary orbit file from ESOC which is also already available. Stay tuned for the news soon. Thanks again! Martin > Martin, Tom, Pascal, ... > > Attached is a zip file containing 1-second S- and X-Band > ODFs from today's DSN tracking of MEX. Each pass is in a > separate file, so there are files from DSS 15, 43, and 63. > There are also two files with 60-s data, probably from > multiple stations and both bands. > > There should be another pair of files tomorrow from the > DSS 14 pass which begins in about three hours and ends at > 0835. > > We expect to hear about profound new discoveries regarding > Phobos shortly. > > Regards, > Dick From susan.c.kurtik@jpl.nasa.gov Thu Mar 4 12:19:02 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion1.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o24KJ2j23011 for ; Thu, 4 Mar 2010 12:19:02 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap02.jpl.nasa.gov [128.149.137.73]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o24KIvl8027264 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Thu, 4 Mar 2010 12:18:57 -0800 Received: from ALTPHYEMBEVSP30.RES.AD.JPL ([172.16.0.31]) by ALTVIREHTSTAP02.RES.AD.JPL ([128.149.137.73]) with mapi; Thu, 4 Mar 2010 12:18:57 -0800 From: "Kurtik, Susan C (9020)" To: "Michel.Denis@esa.int" CC: "owitasse@rssd.esa.int" , "Fred A. Jansen" , "Kern, Albert (9200-Affiliate)" , "Arroyo, Belinda (314E)" , "Kahan, Daniel S (332K)" , !DL-DSN-MPSETD , "Han, Don (343J)" , "Goltz, Gene L (332K)" , "Bell, Julia L (9020)" , "Bracamonte, Larry H" , "mexmps@esa.int" , "Stoloff, Michael J (316E)" , mimsched , "Reboud, Olivier (9210-Affiliate)" , "Simpson, Richard A (6520-Affiliate)" , "Espinueva, Ruben P (314E)" , "Asmar, Sami W (332K)" , "stefan.remus@sciops.esa.int" , "Thompson, Thomas W (3300)" , "Wolfgang.Hell@esa.int" , "Bhanji, Alaudin M (9200)" , "Erickson, James K (9020)" , "Kurtik, Susan C (9020)" , "Mc Namee, John B (9000)" Date: Thu, 4 Mar 2010 12:18:55 -0800 Subject: Re: MEX Phobos flyby 3 March 2010 --- Thanks! Thread-Topic: MEX Phobos flyby 3 March 2010 --- Thanks! Thread-Index: Acq7tJS+KwlemymPQFOehN7cadlsSgAI1UmX Message-ID: In-Reply-To: Accept-Language: en-US Content-Language: en X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/alternative; boundary="_000_C7B555AF8DF72SusanCKurtikjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap02.jpl.nasa.gov [128.149.137.73] X-Source-Sender: susan.c.kurtik@jpl.nasa.gov X-AUTH: Authorized Content-Length: 3792 Status: R --_000_C7B555AF8DF72SusanCKurtikjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable Dear Michel - Thanks so much for your kind words. I have sent this to the DSN teams, they truly appreciate knowing that they have contributed to the success of a mission. Once again, this is an excellent demonstration of the benefits of cross support in enabling space exploration and scientific accomplishments. We are honored to have been able to participate in this support of the Mars Express mission. Best regards, -- Susan C. Kurtik Jet Propulsion Laboratory Deep Space Network Mission Support Manager 818 354-3598 office 818 687-7903 cell Don't leave earth without us On 3/4/10 8:05 AM, "Michel.Denis@esa.int" wrote: Dear DSN and JPL colleagues, Also on behalf of Olivier Witasse (MEX Project Scientist) and Fred Jansen (MEX Mission Manager), we would like to express our warm thanks and congratulations to all the personnel involved in the flawless preparation and execution of the Phobos flyby yesterday. We already heard that the data are of excellent quality and are looking forward to the science results! Kind regards, ------------------------------------------------------------------------ Michel DENIS Head of the MARS EXPRESS Mission Operations Unit ESA / ESOC, Robert-Bosch-Str.5, 64293 DARMSTADT ------------------------------------------------------------------------ From Thomas.W.Thompson@jpl.nasa.gov Fri Mar 5 16:13:19 2010 Return-Path: Received: from mail.jpl.nasa.gov (mailhost.jpl.nasa.gov [128.149.139.105]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o260DGj26059 for ; Fri, 5 Mar 2010 16:13:16 -0800 (PST) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o260CoDh002585 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Fri, 5 Mar 2010 16:12:51 -0800 Received: from ALTPHYEMBEVSP10.RES.AD.JPL ([172.16.0.11]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Fri, 5 Mar 2010 16:12:50 -0800 From: "Thompson, Thomas W (3300)" To: "Carr, Michael H (6021-Affiliate)" , "Kirk, Randolph L (4500-Affiliate)" , "Archinal, Brent (6900-Affiliate)" , "tduxbury@gmu.edu" , "Greeley, Ronald (4010-Affiliate)" , "david.williams@asu.edu" , "james_head_III@brown.edu" , "L.Wilson@lancaster.ac.uk" , "Hiesinger@uni-muenster.de" , "Mccord, Thomas B (4500-Affiliate)" , "jean-philippe_combe@bearfightcenter.com" , "gkramer@bearfightcenter.com" , "squyres@astro.cornell.edu" , "hartmann@psi.edu" , "mchapman@psi.edu" , "Gaetano.DiAchille@lasp.colorado.edu" , "De Jong, Eric M (3223)" , "Zamani, Payam (388B)" , "Plaut, Jeffrey J (3223)" , "Johnson, William T K (3340)" , "Gim, Yonggyu (334D)" , "Ivanov, Anton B (388D-Affiliate)" , "donald-gurnett@uiowa.edu" , "Huff, Richard L (4400-Affiliate)" , "dlk@space.physics.uiowa.edu" , "ddm@space.physics.uiowa.edu" , "estofan@yahoo.com" , "ellen@proxemy.com" , "Milkovich, Sarah M (317D)" , "sandel@arizona.edu" , "KRetherford@swri.edu" , "Atreya, Sushil K (6700-Affiliate)" , "ghansen@rad.ess.washington.edu" , "len.tyler@stanford.edu" , "Simpson, Richard A (6520-Affiliate)" , "Hinson, David P (6700-Affiliate)" , "withers@bu.edu" , "Asmar, Sami W (332K)" , "Holmes, Dwight P (9020)" , "Arroyo, Belinda (314E)" , "Sinha, Mahadeva P (382D)" , "everett.gibson@nasa.gov" , "arvidson@rsmail.wustl.edu" , "John_Mustard@Brown.edu" , "richard.v.morris@nasa.gov" , "clifford@lpi.usra.edu" , "Heggy, Essam (334H)" , "william.farrell@gsfc.nasa.gov" , "leuschen@cresis.ku.edu" , "Phillips, Roger J (6200-Affiliate)" , "watterst@si.edu" , "dwinningham@swri.edu" , "jgluhmann@ssl.berkeley.edu" , "slavney@rsmail.wustl.edu" , "Acton, Charles H (343N)" , "guinness@rsmail.wustl.edu" Date: Fri, 5 Mar 2010 16:12:46 -0800 Subject: Mars Express News - Phobos Flyby Success Thread-Topic: Mars Express News - Phobos Flyby Success Thread-Index: Acq8wb9wk8M1FEfY7Eugp6f+DrE7+w== Message-ID: Accept-Language: en-US Content-Language: en X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/alternative; boundary="_000_C7B6DDFEE68DThomasWThompsonjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: Thomas.W.Thompson@jpl.nasa.gov X-AUTH: Authorized Content-Length: 11409 Status: RO http://www.esa.int/SPECIALS/Mars_Express/SEMIPX6K56G_0.html Phobos Flyby Success European Space Agency 4 March 2010 Mars Express encountered Phobos last night, smoothly skimming past at just 67 km, the closest any manmade object has ever approached Mars' enigmatic moon. The data collected could help unlock the origin of not just Phobos but other "second generation" moons. Something is not right about Phobos. It looks like a solid object but previous flybys have shown that it is not dense enough to be solid all the way through. Instead, it must be 25-35% porous. This has led planetary scientists to believe that it is little more than a "rubble pile" circling Mars. Such a rubble pile would be composed of blocks both large and small resting together, with possibly large spaces between them where they do not fit easily together. Last night's flyby was close enough to give scientists their most exquisite data yet about the gravitational field of Phobos. Mars Express locked onto the radio signal from Earth at around 21:20 CET (20:20 UT). The radio frequency oscillators on the ground are 100 000 times more stable than those on the spacecraft, so for this experiment, which required the best precision possible, the signal was sent up to Mars Express and then returned by the spacecraft to the ground. The radio waves travel at the speed of light and took 6 minutes 34 seconds to travel from Earth to the spacecraft last night. So the round trip time was 13 minutes 8 seconds. Once the signal was received back at Earth, it was clearly strong and good. So strong that radio amateurs were also able to lock onto the signal, although their equipment would not be able to detect the subtle variations induced by the gravity of Phobos. Now that the data are all collected, the analysis can begin.First will be an estimate of the density variation across the moon. This will tell scientists just how much of Phobos' interior is likely to be composed of voids. "Phobos is probably a second-generation Solar System object," says Martin Paetzold, Universitat Koln, Cologne, Germany, and Principal Investigator of the Mars Radio Science (MaRS) experiment. Second generation means that it coalesced in orbit after Mars formed, rather than forming concurrently out of the same birth cloud as the Red Planet. There are other moons around other planets where this is thought to have been the case too, such as Amalthea around Jupiter. Whatever the precise origin, Phobos will eventually crumble back into this disrupted state. It is gradually spiralling towards Mars and will eventually be pulled apart. "It came from debris, it will return to debris," says Paetzold. In the meantime, it is there to be studied and explored. Last night's flyby was just one of a campaign of 12 Mars Express flybys taking place in February and March 2010. For the previous two, the radar was working, attempting to probe beneath the surface of the moon, looking for reflections from structures inside. In the coming flybys, the Mars Express camera will take over, providing high resolution pictures of the moon's surface. More information Updates as the flybys continue will be posted on the Mars Express blog . Contacts for editors: Martin Patzold Principal Investigator of the Mars Radio Science (MaRS) experiment Universitat Koln, Germany Email: mpaetzol@uni-koeln.de Olivier Witasse ESA Project Scientist Mars Express ESTEC, The Netherlands Email: owitasse@rssd.esa.int From Thomas.W.Thompson@jpl.nasa.gov Wed Mar 17 13:49:26 2010 Return-Path: Received: from mail.jpl.nasa.gov (sentrion2.jpl.nasa.gov [128.149.139.106]) by magellan.stanford.edu (8.11.7p3+Sun/8.11.7) with ESMTP id o2HKnQj21354 for ; Wed, 17 Mar 2010 13:49:26 -0700 (PDT) Received: from mail.jpl.nasa.gov (altvirehtstap01.jpl.nasa.gov [128.149.137.72]) by smtp.jpl.nasa.gov (Switch-3.4.2/Switch-3.4.1) with ESMTP id o2HKmo2l017524 (using TLSv1/SSLv3 with cipher RC4-MD5 (128 bits) verified FAIL); Wed, 17 Mar 2010 13:48:50 -0700 Received: from ALTPHYEMBEVSP10.RES.AD.JPL ([172.16.0.11]) by ALTVIREHTSTAP01.RES.AD.JPL ([128.149.137.72]) with mapi; Wed, 17 Mar 2010 13:48:49 -0700 From: "Thompson, Thomas W (3300)" Date: Wed, 17 Mar 2010 13:48:47 -0700 Subject: Mars News - Mars Express - Phobos flyby images Thread-Topic: Mars News - Mars Express - Phobos flyby images Thread-Index: AcrGEz1iWSsimAI7p0eqiRy0nA9i2w== Message-ID: Accept-Language: en-US Content-Language: en X-MS-Has-Attach: X-MS-TNEF-Correlator: acceptlanguage: en-US Content-Type: multipart/alternative; boundary="_000_C7C68E3FEA06ThomasWThompsonjplnasagov_" MIME-Version: 1.0 X-Source-IP: altvirehtstap01.jpl.nasa.gov [128.149.137.72] X-Source-Sender: Thomas.W.Thompson@jpl.nasa.gov X-AUTH: Authorized Content-Length: 9750 Status: RO --_000_C7C68E3FEA06ThomasWThompsonjplnasagov_ Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=3D46710 Phobos flyby images European Space Agency 15 Mar 2010 Images from the recent flyby of Phobos, on 7 March 2010, are released today. The images show Mars' rocky moon in exquisite detail, with a resolution of just 4.4 metres per pixel. They show the proposed landing sites for the forthcoming Phobos-Grunt mission. (This article was originally posted on the ESA Space Science Portal .) ESA's Mars Express spacecraft orbits the Red Planet in a highly elliptical, polar orbit that brings it close to Phobos every five months. It is the only spacecraft currently in orbit around Mars whose orbit reaches far enough from the planet to provide a close-up view of Phobos. Like our Moon, Phobos always shows the same side to the planet, so it is only by flying outside the orbit that it becomes possible to observe the far side. Mars Express did just this on 7, 10 and 13 March 2010. Mars Express also collected data with other instruments. Phobos is an irregular body measuring some 27 x 22 x 19 km. Its origin is debated. It appears to share many surface characteristics with the class of 'carbonaceous C-type' asteroids, which suggests it might have been captured from this population. However, it is difficult to explain either the capture mechanism or the subsequent evolution of the orbit into the equatorial plane of Mars. An alternative hypothesis is that it formed around Mars, and is therefore a remnant from the planetary formation period. In 2011 Russia will send a mission called Phobos-Grunt (meaning Phobos Soil) to land on the martian moon, collect a soil sample and return it to Earth for analysis. For operational and landing safety reasons, the proposed landing sites were selected on the far side of Phobos within the area 5=C2=B0S-5=C2=B0N, 230-235=C2=B0E. This region was imaged by the HRSC high-resolution camera o= f Mars Express during the July-August 2008 flybys of Phobos. But new HRSC images showing the vicinity of the landing area under different conditions, such as better illumination from the Sun, remain highly valuable for mission planners. It is expected that Earth-based ESA stations will take part in controlling Phobos-Grunt, receiving telemetry and making trajectory measurements, including implementation of very long-baseline interferometry (VLBI). This cooperation is realized on the basis of the agreement on collaboration of the Russian Federal Space Agency and ESA in the framework of the 'Phobos-Grunt' and 'ExoMars' projects. Mars Express will continue to encounter Phobos until the end of March, when the moon will pass out of range. During the remaining flybys, HRSC and other instruments will continue to collect data. *More information* Univ.-Prof. Dr. Gerhard Neukum Freie Universitaet Berlin Mobile: +49 171-7647177 Tel: +49 30 838 70579; +49 30 838 70575 Email: gneukumzedat.fu-berlin.de Prof. Dr. Ralf Jaumann German Aerospace Center Phone: +49 30 67055-400 Fax: +49 30 67055-402 Email: ralf.jaumanndlr.de Olivier Witasse, ESA Mars Express project scientist ESTEC, The Netherlands Email: owitasserssd.esa.int Updates as the flybys take place will be posted on the Mars Express blog (see link in right-hand menu). *Note to editors* The High Resolution Stereo Camera (HRSC) experiment on the ESA Mars Express mission is led by the Principal Investigator (PI) Prof. Dr. Gerhard Neukum, who also designed the camera. The science team of the experiment consists of 45 Co-Investigators from 32 institutions and 10 nations. The camera was developed at the German Aerospace Center (DLR) under the leadership of the PI and built in cooperation with industrial partners (EADS Astrium, Lewicki Microelectronic GmbH and Jena-Optronik GmbH). HRSC is operated by the DLR Institute of Planetary Research, through ESA/ESOC. The science planning coordination between all instruments is performed at ESA/ESAC. The systematic processing of the HRSC image data is carried out at DLR. The scenes shown here were processed by the PI group at the Institute for Geosciences of the Freie Universitaet Berlin in cooperation with DLR, Institute of Planetary Research, Berlin.