<?xml version="1.0" encoding="UTF-8"?>
<?xml-model href="http://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1400.sch" 
   schematypens="http://purl.oclc.org/dsdl/schematron"?>
<Product_Context 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 
     http://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1400.xsd 
   ">
   <Identification_Area>
      <logical_identifier>urn:nasa:pds:context:instrument_host:spacecraft.maven</logical_identifier>
      <version_id>1.0</version_id>
      <title>MAVEN</title>
      <information_model_version>1.4.0.0</information_model_version>
      <product_class>Product_Context</product_class>
      <Alias_List>
         <Alias>
            <alternate_id>MVN</alternate_id>
         </Alias>
      </Alias_List>
      <Modification_History>
         <Modification_Detail>
            <modification_date>2015-03-16</modification_date>
            <version_id>1.0</version_id>
            <description>
               Initial version.
            </description>
         </Modification_Detail>
      </Modification_History>
   </Identification_Area>
   <Reference_List>
<!-- Add reference MAVEN spacecraft description paper when available      
      <External_Reference>
         <doi></doi>
         <reference_text></reference_text>
         <description></description>
      </External_Reference>
-->
   </Reference_List>
   <Instrument_Host>
      <type>Spacecraft</type>
      <description>
         The MAVEN mission launched on an Atlas V November 18, 2013. After a ten-month ballistic cruise 
         phase, Mars orbit insertion occurred on September 22, 2014. Following a 5-week transition phase, the 
         spacecraft began orbiting Mars at a 75 inclination, with a 4.5 hour period and periapsis altitude of 
         140-170 km (density corridor of 0.05-0.15 kg/km3). Over a one-Earth-year period, periapsis will 
         precess over a wide range of latitude and local time, while MAVEN obtains detailed measurements of 
         the upper atmosphere, ionosphere, planetary corona, solar wind, interplanetary/Mars magnetic fields, 
         solar EUV and solar energetic particles, thus defining the interactions between the Sun and Mars. 
         MAVEN will explore down to the homopause during a series of five 5-day “deep dip” campaigns for which 
         periapsis will be lowered to an atmospheric density of 2 kg/km3 (~125 km altitude) in order to sample 
         the transition from the collisional lower atmosphere to the collisionless upper atmosphere. These five 
         campaigns will be interspersed though the mission to sample the subsolar region, the dawn and dusk 
         terminators, the anti-solar region, and the north pole.
      </description>
   </Instrument_Host>
</Product_Context>