PDS_VERSION_ID               = PDS3
RECORD_TYPE                  = STREAM
STANDARD_DATA_PRODUCT_ID     = HEA
DATA_SET_ID                  =  "MEX-X-MRS-1/2/3-EXT2-1719-V1.0"
PRODUCT_ID                   = "M00SUE0L1A_HEA_083630940_00.TXT"
PRODUCT_CREATION_TIME        =  2012-01-23T16:37:10.000
PRODUCER_ID                  = "SUE"
INSTRUMENT_HOST_ID           = "MEX"
OBJECT                       = TEXT
PUBLICATION_DATE               = 2009-01-06
NOTE                           = "DSN MEX Data Collection"
END_OBJECT                   = TEXT
END


Miscellaneous
=============

     This is the first report since HEA8357A.TXT.


Open Loop Data
==============

  Data Collection
  ---------------

     We have completed quick-look processing on the following MEX RSR open
loop solar conjunction data at Stanford:

DOY DSS        RSR        BAND RSR CH KSPS BT  REC   RECS      RSR      MAX
          START    STOP         ID         RS  LEN          FILE NAME   SNR
--- --- -------- -------- ---- --- -- ---- -- ----- ----- ------------ -----
353  65 11:00:00 15:14:59 X/XR   3  1    2 16  8260 15300 8353110A.RSR  49.1
353  65 12:05:00 14:55:00 X/SR   4  1    2 16  8260 10201 8353120B.RSR  30.5
354  15 19:16:01 21:40:00 X/XR   3  1    2 16  8260  8640 8354191A.RSR  49.3
354  15 19:40:01 21:19:59 X/SR   4  1    2 16  8260  5999 8354194B.RSR  32.6
356  65 10:35:00 14:22:00 X/XR   3  1    2 16  8260 13621 8356103A.RSR  48.0
356  65 11:23:00 14:22:00 X/SR   4  1    2 16  8260 10741 8356112B.RSR  31.7
357  65 10:00:00 15:15:00 X/XR   3  1    2 16  8260 18901 8357100A.RSR  48.3
357  65 10:55:00 11:56:00 X/SR   4  1    2 16  8260  3661 8357105B.RSR  31.8
362  65 10:30:00 15:09:59 X/XR   3  1    2 16  8260 16800 8362103A.RSR  47.6
362  65 11:18:00 14:55:00 X/SR   4  1    2 16  8260 13021 8362111B.RSR  32.8
363  65 09:40:00 15:10:00 X/XR   3  1    2 16  8260 19801 8363094A.RSR  47.7
363  65 10:43:00 14:55:00 X/SR   4  1    2 16  8260 15121 8363104B.RSR  31.6
364  15 15:40:00 20:57:00 X/XR   3  1    2 16  8260 19021 8364154A.RSR  48.7
364  15 16:40:00 20:42:00 X/SR   4  1    2 16  8260 14521 8364164B.RSR  34.2
366  63 10:25:00 14:04:59 X/XR   1  1    2 16  8260 13200 8366102A.RSR  56.6
366  63 11:11:00 13:20:00 X/SR   3  1    2 16  8260  7741 8366111B.RSR  40.2
366  63 10:25:00 14:04:59 X/XL   2  1    2 16  8260 13200 8366102C.RSR  27.2
366  63 11:11:00 13:20:00 X/SL   4  1    2 16  8260  7741 8366111D.RSR  40.2
005  14 18:55:00 22:50:00 X/XR   3  1    2 16  8260 14101 9005185A.RSR  56.9
005  14 19:48:00 22:35:00 X/SR   4  1    2 16  8260 10021 9005194B.RSR  40.9

  Anomalies
  ---------

     All data appear to have been collected with X-Band telemetry modulation
on.  Compared with the most recent bistatic radar (August 2008 at 2.36 AU),
the carrier to noise level here (2.42 AU) is about 7 dB lower when expectation
is only 0.2 dB lower.

     On 2008/366 the channel supposedly carrying S-LCP appears to have only
a copy of the S-RCP signal.

     So far as planning is concerned, these data were collected for gravity
studies; but the real application is to solar corona studies.  "Gravity" was
used to obtain the desired spacecraft and ground configurations without having
to define a new instrument mode.