PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM DATA_SET_ID = "MEX-X-MRS-1/2/3-EXT5-3796-V1.0" STANDARD_DATA_PRODUCT_ID = ENB PRODUCER_ID = "SUE" PRODUCT_ID = "M00SUE0L1A_ENB_151951255_00.TXT" PRODUCT_CREATION_TIME = 2017-10-05T13:51:21.000 INSTRUMENT_HOST_ID = "MEX" OBJECT = TEXT PUBLICATION_DATE = 2016-01-28 NOTE = "MEX SUE Experimenter Notes" END_OBJECT = TEXT END From daniel.s.kahan@jpl.nasa.gov Tue Jul 14 10:16:10 2015 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 t6EHG9p24148 for ; Tue, 14 Jul 2015 10:16:09 -0700 (PDT) Received: from mail.jpl.nasa.gov (ap-ehub-sp01.jpl.nasa.gov [128.149.137.148]) by smtp.jpl.nasa.gov (Sentrion-MTA-4.3.1/Sentrion-MTA-4.3.1) with ESMTP id t6EHG8Ka023706 (using TLSv1 with cipher AES128-SHA (128 bits) verified NO); Tue, 14 Jul 2015 10:16:08 -0700 Received: from AP-EMBX-SP20.RES.AD.JPL ([169.254.8.135]) by ap-ehub-sp01.RES.AD.JPL ([169.254.3.196]) with mapi id 14.03.0210.002; Tue, 14 Jul 2015 10:16:07 -0700 From: "Kahan, Daniel S (332K)" To: "Simpson, Richard A (6020-Affiliate)" , "Matthias.Hahn@uni-koeln.de" Subject: MEX 2015-195 Solar Corona Data Thread-Topic: MEX 2015-195 Solar Corona Data Thread-Index: AdC+WCz/kRX5VBSgRuytLSJr96VHqg== Date: Tue, 14 Jul 2015 17:16:06 +0000 Message-ID: <9FB7C98ED504AC408404AC9B54B855734D4266E0@ap-embx-sp20.RES.AD.JPL> Accept-Language: en-US Content-Language: en-US X-MS-Has-Attach: X-MS-TNEF-Correlator: x-originating-ip: [128.149.137.26] Content-Type: multipart/alternative; boundary="_000_9FB7C98ED504AC408404AC9B54B855734D4266E0apembxsp20RESAD_" MIME-Version: 1.0 X-Source-Sender: daniel.s.kahan@jpl.nasa.gov X-AUTH: Authorized Content-Length: 12631 --_000_9FB7C98ED504AC408404AC9B54B855734D4266E0apembxsp20RESAD_ Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: quoted-printable Dick, Matthias, A MEX Solar Corona Observation was conducted at DSS-63 on 2015-195. RSR ope= n-loop data were recorded and played back as follows: - X-band RCP, 2-way - RSR2B1 - 2 kHz, 16 bits - start =3D 12:55:01 - stop =3D 14:59:00 - SNR =3D ~59 dB-Hz and: - S-band RCP, 2-way - RSR1B1 - 2 kHz, 16 bits - start =3D 12:55:01 - stop =3D 14:59:00 - SNR =3D ~40 dB-Hz plus: - X-band LCP, 2-way - RSR2A1 - 2 kHz, 16 bits - start =3D 12:55:01 - stop =3D 14:59:00 - SNR =3D ~33 dB-Hz and: - S-band LCP, 2-way - RSR1A1 - 2 kHz, 16 bits - start =3D 12:55:01 - stop =3D 14:59:00 - SNR =3D ~23 dB-Hz These data are now available in ~rsimpson/MEX on rsops2 and /SCO/RSR/2015 o= n Saturn. The above SNR values are roughly the highest values seen during t= he track. Regards, Danny