PDS_VERSION_ID                    = PDS3  /* Version 3.8 February 27, 2009 */
RECORD_TYPE                       = STREAM
LABEL_REVISION_NOTE               = "
  2024-06-01 JUNO: Sarkissian Revision 1"

OBJECT                  = DATA_SET
  DATA_SET_ID             = "JNO-J-MWR-5-ATM-BRIGHT-TEMP-VS-LAT-V1.0"

  OBJECT                  = DATA_SET_INFORMATION
    DATA_SET_NAME           = "
      JUNO JUPITER MWR ATMOSPHERIC BRIGHTNESS TEMPERATURE V1.0"
    DATA_SET_COLLECTION_MEMBER_FLG = "N"
    DATA_OBJECT_TYPE        = FILE
    ARCHIVE_STATUS          = "ARCHIVED - NONACCUMULATING"
    START_TIME              = 2016-07-06T20:00:00
    STOP_TIME               = NULL
    DATA_SET_RELEASE_DATE   = NULL
    PRODUCER_FULL_NAME      = "DR. STEVEN M. LEVIN"
    DETAILED_CATALOG_FLAG   = "N"
    DATA_SET_TERSE_DESC     = "
      This dataset includes Juno MWR ATMOSPHERIC BRIGHTNESS TEMPERATURE
      (and their angular dependence) as a function of latitude."

    ABSTRACT_DESC           = "
      The Juno MWR ATMOSPHERIC BRIGHTNESS TEMPERATURE dataset in this
      volume is a nonaccumulating dataset derived from high-rate perijove
      data. The atmospheric brightness temperature (and their angular
      dependence) is provided as a function of planetocentric latitude.
      The data is store is several product files separated by MWR channel
      and perijove."


    CITATION_DESC           = "LEVIN, S. M.,
      JUNO JUPITER MWR ATMOSPHERIC BRIGHTNESS TEMPERATURE V1.0,
      JNO-J-MWR-5-ATM-BRIGHT-TEMP-VS-LAT-V1.0, NASA Planetary Data System,
      2024."

    DATA_SET_DESC           = "

      Data Set Overview
      =================
      The Juno MWR ATMOSPHERIC BRIGHTNESS TEMPERATURE dataset is a
      nonaccumulating dataset derived from high-rate perijove data from the
      orbital phase of the Juno mission. The dataset may get updated based
      on new information from new perijove data. The brightness temperature
      data and their angular dependency are provided as a function of
      planetocentric latitude. The atmospheric brightness temperature and
      other related data are organized in several files by MWR channel and
      perijove.

      The product files in this dataset are text files in CSV format.


      Parameters
      ==========
      TBD


      Processing
      ==========
      The data included in this volume set is produced by MWR IOT as
      described in section 2.3 of the VOLSIS document found under the
      DOCUMENTS subdirectory. The algorithm/process used in the computation
      of atmospheric brightness temperature is given in Oyafuso et al.
      (2020), (https://doi.org/10.1029/2020EA001254 also OYAFUSO_ETAL_2020
      document found under the DOCUMENTS subdirectory).


      Data
      ====
      A complete product from a perijove consists of six files. The data
      from MWR six channels are stored in separate files. In the files, the
      data are organized in rows in the increasing order of planetocentric
      latitudee. The details of the products and the formatting of the files
      are described in Section 6.3, Section 7.6, and Appendix E.10 of the
      VOLSIS document found under the DOCUMENTS subdirectory.


      Ancillary Data
      ==============
      This data set is complete and requires no ancillary data for its
      interpretation.


      Coordinate Systems
      ==================
      The coordinate system associated with this product is Jupiter
      planetocentric latitude. The recorded coordinate is determined from
      SPICE utilities.


      Software
      ========
      No software is provided to view, interpret, or convert this data set.
      All files are in ASCII format, however, and are readily readible 
      through standard programs such as textedit, Microwave Excel and Word, 
      etc.
      
      
      Media/Format
      ============
      This data set is provided to the Planetary Data System by the Juno 
      Science Operation Center (JSOC) as described in section 5.2 of the 
      VOLSIS document found under the DOCUMENTS subdirectory."


    CONFIDENCE_LEVEL_NOTE   = "
        
      Confidence Level Overview
      =========================
      TBD  

      
      Review
      ======
      The MWR calibrated complete data will be reviewed internally by the 
      Juno MWR instrument team prior to release to the PDS.  The data set 
      will also be reviewed by the PDS.
      

      Data Coverage and Quality
      =========================
      TBD

      
      Limitations
      ===========
      The use of the data in JNO-J-MWR-5-ATM-BRIGHT-TEMP-VS-LAT-V1.0
      dataset should be limited to [-60deg, +60deg] latitude interval. That is 
      primarily because the assumption of longitudinal invariance becomes
      less reasonable toward the poles: instead of assuming constant thermal
      properties over compact, rectangular patches of limited latitude and
      longitude ranges, the regions become annuli encompassing a very large
      range of longitudes.  A secondary reason is that the early perijoves
      were at low latitudes and deconvolution at high latitudes had a much
      larger uncertainty due to the greater distance from the planet and
      attendant larger footprint size.
      
      More limitations on the dataset may be defined as the MWR team gains
      experience operating the instrument in flight conditions."
      
  END_OBJECT              = DATA_SET_INFORMATION
  
    
  OBJECT                  = DATA_SET_TARGET
    TARGET_NAME             = "JUPITER"
  END_OBJECT              = DATA_SET_TARGET

  OBJECT                  = DATA_SET_HOST
    INSTRUMENT_HOST_ID      = "JNO"
    INSTRUMENT_ID           = "MWR"
  END_OBJECT              = DATA_SET_HOST
  
  OBJECT                  = DATA_SET_MISSION
    MISSION_NAME            = "JUNO"
  END_OBJECT              = DATA_SET_MISSION
  
  OBJECT                  = DATA_SET_REFERENCE_INFORMATION
     REFERENCE_KEY_ID        = "NULL"
  END_OBJECT              = DATA_SET_REFERENCE_INFORMATION
  
END_OBJECT              = DATA_SET
END