PDS_VERSION_ID               = PDS3
RECORD_TYPE                  = STREAM
DATA_SET_ID                  =  "MEX-X-MRS-1/2/3-EXT5-3794-V1.0"
STANDARD_DATA_PRODUCT_ID     = ENB
PRODUCER_ID                  = "SUE"
PRODUCT_ID                   = "M00SUE0L1A_ENB_151931158_00.TXT"
PRODUCT_CREATION_TIME        =  2017-10-05T13:27:21.000
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 Mon Jul 13 10:38:31 2015
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From: "Kahan, Daniel S (332K)" <daniel.s.kahan@jpl.nasa.gov>
To: "Simpson, Richard A (6020-Affiliate)" <rsimpson@magellan.stanford.edu>,
        "Matthias.Hahn@uni-koeln.de" <Matthias.Hahn@uni-koeln.de>
Subject: MEX 2015-193 Solar Corona Data
Thread-Topic: MEX 2015-193 Solar Corona Data
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Date: Mon, 13 Jul 2015 17:38:28 +0000
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Dick, Matthias,

A MEX Solar Corona Observation was conducted at DSS-65 on 2015-193. RSR ope=
n-loop data were recorded and played back as follows:

    -  X-band RCP, 2-way
    -  RSR1B1
    -  2 kHz, 16 bits
    -  start =3D 11:58:01
    -  stop =3D 14:04:00
    -  SNR =3D ~50 dB-Hz

  and:

    -  S-band RCP, 2-way
    -  RSR1A1
    -  2 kHz, 16 bits
    -  start =3D 11:58:01
    -  stop =3D 14:04:00
    -  SNR =3D ~33 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