PDS_VERSION_ID               = PDS3
RECORD_TYPE                  = STREAM
STANDARD_DATA_PRODUCT_ID     = HEA
DATA_SET_ID                  =  "MEX-M-MRS-1/2/3-EXT2-1516-V1.0"
PRODUCT_ID                   = "M00SUE0L1A_HEA_082181944_00.TXT"
PRODUCT_CREATION_TIME        =  2011-07-21T17:11:43.000
PRODUCER_ID                  = "SUE"
INSTRUMENT_HOST_ID           = "MEX"
OBJECT                       = TEXT
PUBLICATION_DATE               = 2008-08-14
NOTE                           = "DSN MEX Occultation Data"
END_OBJECT                   = TEXT
END


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

     This is the first report since HEA8226A.TXT.  It reports on processing
of occultation data from 2008/218, which were noted as maving been missed in
HEA8226A.TXT.


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

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

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

DOY DSS        RSR        BAND RSR CH KSPS BT  REC   RECS      RSR      MAX
          START    STOP         ID         RS  LEN          FILE NAME   SNR
--- --- -------- -------- ---- --- -- ---- -- ----- ----- ------------ -----
218  15 19:44:00 20:05:00 X/XR   6  1    2 16  8260  1261 8218194A.RSR  56.3
218  15 19:44:00 20:05:00 X/SR   5  1    2 16  8260  1261 8218194B.RSR  35.4

     With the exception of low-level square wave modulation on the carrier
amplitude, these appear to be excellent data.  The square wave modulation was
noted in HEA8226A.TXT; the data from day 218 have the most pronounced
modulation (approaching 0.5 dB peak-to-peak) since the current occultation
season began.