PDS_VERSION_ID               = PDS3
RECORD_TYPE                  = STREAM
STANDARD_DATA_PRODUCT_ID     = HEA
DATA_SET_ID                  =  "MEX-X-MRS-1/2/3-EXT5-3776-V1.0"
PRODUCT_ID                   = "M00SUE0L1A_HEA_151730928_00.TXT"
PRODUCT_CREATION_TIME        =  2017-09-27T13:47:00.000
PRODUCER_ID                  = "SUE"
INSTRUMENT_HOST_ID           = "MEX"
OBJECT                       = TEXT
PUBLICATION_DATE               = 2015-06-30
NOTE                           = "MEX/DSN SCO Data Report"
END_OBJECT                   = TEXT
END


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

     This is the first report since HEAF168A.TXT.


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

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

     We have transferred the following MEX RSR open loop solar conjunction
data to Stanford:

DOY DSS        RSR        BAND RSR CH KSPS BT  REC   RECS      RSR      MAX
          START    STOP         ID         RS  LEN          FILE NAME   SNR
--- --- -------- -------- ---- --- -- ---- -- ----- ----- ------------ -----
169  14 22:48:01 01:59:00 X/XR   6  1    2 16  8260 11460 F169224A.RSR  60.
169  14 22:48:01 01:59:00 X/SR   2  1    2 16  8260 11460 F169224B.RSR  35.
169  14 22:48:01 01:59:00 X/XL   5  1    2 16  8260 11460 F169224C.RSR  40.
169  14 22:48:01 01:59:00 X/SL   1  1    2 16  8260 11460 F169224D.RSR  10.
170  63 07:43:01 15:54:00 X/XR   4  1    2 16  8260 29460 F170074A.RSR  60.
170  63 07:43:01 15:54:00 X/SR   2  1    2 16  8260 29460 F170074B.RSR  42.
170  63 07:43:01 15:54:00 X/XL   3  1    2 16  8260 29460 F170074C.RSR  45.
170  63 07:43:01 15:54:00 X/SL   1  1    2 16  8260 29460 F170074D.RSR  24.
171  14 15:03:01 22:24:00 X/XR   6  1    2 16  8260 26460 F171150A.RSR  60.
171  14 15:03:01 22:24:00 X/SR   2  1    2 16  8260 26460 F171150B.RSR  45.
171  14 15:03:01 22:23:59 X/XL   5  1    2 16  8260 26459 F171150C.RSR  40.
171  14 15:03:01 22:24:00 X/SL   1  1    2 16  8260 26460 F171150D.RSR  25.
172  63 09:48:01 16:59:00 X/XR   4  1    2 16  8260 25860 F172094A.RSR  60.
172  63 09:48:01 16:59:00 X/SR   2  1    2 16  8260 25860 F172094B.RSR  46.
172  63 09:48:01 16:59:00 X/XL   3  1    2 16  8260 25860 F172094C.RSR  43.
172  63 09:48:01 16:59:00 X/SL   1  1    2 16  8260 25860 F172094D.RSR  27.
173  63 09:28:01 13:39:00 X/XR   4  1    2 16  8260 15060 F173092A.RSR  60.
173  63 09:28:01 13:39:00 X/SR   2  1    2 16  8260 15060 F173092B.RSR  47.
173  63 09:28:01 13:39:00 X/XL   3  1    2 16  8260 15060 F173092C.RSR  43.
173  63 09:28:01 13:39:00 X/SL   1  1    2 16  8260 15060 F173092S.RSR  30.
174  63 11:48:01 17:39:00 X/XR   4  1    2 16  8260 21060 F174114A.RSR  60.
174  63 11:48:01 17:39:00 X/SR   2  1    2 16  8260 21060 F174114B.RSR  45.
174  63 11:48:01 17:39:00 X/XL   3  1    2 16  8260 21060 F174114C.RSR  40.
174  63 11:48:01 17:39:00 X/SL   1  1    2 16  8260 21060 F174114D.RSR  25.
176  43 23:33:01 05:34:00 X/XR   4  1    2 16  8260 21660 F176233A.RSR  58.
176  43 23:33:01 05:34:00 X/SR   2  1    2 16  8260 21660 F176233B.RSR  45.
176  43 23:33:01 05:34:00 X/XL   3  1    2 16  8260 21660 F176233C.RSR  34.
176  43 23:33:01 05:34:00 X/SL   1  1    2 16  8260 21660 F176233D.RSR  23.

     Because Stanford's software is in transitiion, we do not currently
have a way to check data quality (e.g., maximum SNR and plots of data).
The MAX SNR values listed above are from Danny Kahan's inspection of the
data before they were transferred to Stanford.

     Additional passes are scheduled for SCO over the next four weeks;
but most will be RCP only using 34-m antennas.