<?xml version="1.0" encoding="UTF-8" standalone="no"?>

<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1E00.sch" schematypens="http://purl.oclc.org/dsdl/schematron"?>

<Product_Observational xmlns="http://pds.nasa.gov/pds4/pds/v1" 
  xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" 
  xsi:schemaLocation="http://pds.nasa.gov/pds4/pds/v1 https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1E00.xsd">
  <Identification_Area>
    <logical_identifier>urn:nasa:pds:lp_rs_jpl_gravity_derived:data_ascii:jbl070d1_ascii</logical_identifier>
    <version_id>1.0</version_id>
    <title>Lunar Prospector Gravity File: jbl070d1_ascii</title>
    <information_model_version>1.14.0.0</information_model_version>
    <product_class>Product_Observational</product_class>
    <Modification_History>
      <Modification_Detail>
        <modification_date>2021-01-14</modification_date>
        <version_id>1.0</version_id>
        <description>PDS4 migrated product.</description>
      </Modification_Detail>
    </Modification_History>
  </Identification_Area>
  <Observation_Area>
    <Time_Coordinates>
      <start_date_time xsi:nil="true" nilReason="missing"></start_date_time>
      <stop_date_time xsi:nil="true" nilReason="missing"></stop_date_time>
    </Time_Coordinates>
    <Investigation_Area>
      <name>Lunar Prospector</name>
      <type>Mission</type>
      <Internal_Reference>
        <lid_reference>urn:nasa:pds:context:investigation:mission.lunar_prospector</lid_reference>
        <reference_type>data_to_investigation</reference_type>
      </Internal_Reference>
    </Investigation_Area>
    <Observing_System>
      <Observing_System_Component>
        <name>Lunar Prospector</name>
        <type>Host</type>
        <Internal_Reference>
          <lid_reference>urn:nasa:pds:context:instrument_host:spacecraft.lp</lid_reference>
          <reference_type>is_instrument_host</reference_type>
        </Internal_Reference>
      </Observing_System_Component>
      <Observing_System_Component>
        <name>Radio Science Subsystem</name>
        <type>Instrument</type>
        <Internal_Reference>
          <lid_reference>urn:nasa:pds:context:instrument:lp.rss</lid_reference>
          <reference_type>is_instrument</reference_type>
        </Internal_Reference>
      </Observing_System_Component>
    </Observing_System>   
    <Target_Identification>
      <name>Moon</name>
      <type>Satellite</type>
      <Internal_Reference>
        <lid_reference>urn:nasa:pds:context:target:satellite.earth.moon</lid_reference>
        <reference_type>data_to_target</reference_type>
      </Internal_Reference>
    </Target_Identification>
  </Observation_Area>
  <Reference_List>
    <Internal_Reference>
      <lid_reference>urn:nasa:pds:lp_rs_jpl_gravity_derived:data_image:jbl070d1_img</lid_reference>
      <reference_type>data_to_associate</reference_type>
    </Internal_Reference>
  </Reference_List>

  <File_Area_Observational>
    <File>
      <file_name>jbl070d1.dat</file_name>
      <comment>
        This file contains a digital,
        1 X 1 degree resolution grid of Bouguer gravity anomalies of
        the moon. It is a 360 x 180 grid from 89.5 to -89.5 degrees
        latitude, and -180.0 to 179.0 degrees longitude.  The observation is
        Bouguer vertical gravity in milligals at the surface referenced to a
        sphere of 1738.0 km radius. The Bouguer anomaly is the observed gravity
        as given by the indicated gravity model minus the theoretical gravity
        from the topography model. A crustal density of 2.8 and mean density of
        3.34 gm/cm^3 are used together with the GLTM-2C 90th degree and order
        topography model (Smith et. al., 1997, Topography of the Moon from the
        Clementine Lidar, Journal of Geophysical Research, 102, 1591-1611) to
        determine the theoretical gravity. The degree one terms are not included
        and there is no correction for maria fill. The method of computing the
        theoretical gravity of a topography model was done by expanding in powers
        (Wieczorek and Phillips, 1998, Potential Anomalies on a Sphere:
        Applications to the Lunar Crust, Journal of Geophysical Research, 103,
        1715-1724). The anomaly may be from a truncation in degree of a
        delivered gravity field. The naming convention for the degree used
        is, e.g., JBL070D where 70 indicates the maximum degree of the gravity
        field used to create the grid.
        
        This is a 2-D grid of the Bouguer gravity
        anomalies of the Moon in milligals (1 milligal = 0.01 mm/s/s). The
        file contains 180 blocks of 36 records, with each record containing
        10 Bouguer anomaly values plus an ASCII carriage-return line-feed
        pair as a delimiter. The first block contains values at 89.5N latitude;
        the first value in the first record is the Bouguer anomaly at
        (89.5N, 180.0W).
      </comment>
    </File>
    
    <Stream_Text>
      <offset unit="byte">0</offset>
      <parsing_standard_id>7-Bit ASCII Text</parsing_standard_id>
      <record_delimiter>Carriage-Return Line-Feed</record_delimiter>
    </Stream_Text>
  </File_Area_Observational>

  <File_Area_Observational_Supplemental>
    <File>
      <file_name>jbl070d1.lbl</file_name>
    </File>
    <Stream_Text>
      <offset unit="byte">0</offset>
      <parsing_standard_id>PDS3</parsing_standard_id>
      <description>Original PDS3 label</description>
      <record_delimiter>Carriage-Return Line-Feed</record_delimiter>
    </Stream_Text>
  </File_Area_Observational_Supplemental>
</Product_Observational>
