<?xml version="1.0" encoding="UTF-8"?>
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1700.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 https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1700.xsd">
    
    <Identification_Area>
        <logical_identifier>urn:nasa:pds:context:instrument_host:spacecraft.sakig</logical_identifier>
        <version_id>1.0</version_id>
        <title>SAKIGAKE</title>
        <information_model_version>1.7.0.0</information_model_version>
        <product_class>Product_Context</product_class>
        <Modification_History>
            <Modification_Detail>
                <modification_date>2016-10-01</modification_date>
                <version_id>1.0</version_id>
                <description>
                    extracted metadata from PDS3 catalog and
                    modified to comply with PDS4 Information Model
                </description>
            </Modification_Detail>
        </Modification_History>
    </Identification_Area>

    <Reference_List>
        <Internal_Reference>
            <lidvid_reference>urn:nasa:pds:context:investigation:mission.sakigake::1.0</lidvid_reference>
            <reference_type>instrument_host_to_investigation</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lidvid_reference>urn:nasa:pds:context:instrument:imf.sakig::1.0</lidvid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
        <Internal_Reference>
            <lidvid_reference>urn:nasa:pds:context:instrument:sow.sakig::1.0</lidvid_reference>
            <reference_type>instrument_host_to_instrument</reference_type>
        </Internal_Reference>
<!--        <Internal_Reference> -->
<!--            <lidvid_reference>urn:nasa:pds:context:target:comet.halley::1.0</lidvid_reference> -->
<!--            <reference_type>instrument_host_to_target</reference_type> -->
<!--        </Internal_Reference> -->
        <External_Reference>
            <reference_text>
                   Reinhard, R and B. Battrick (eds), &apos;Space Missions to Halley&apos;s Comet&apos;, European
                   Space Agency ESA SP-1066, ESA Pub Div, Moordwijk, Netherlands, 1986.
            </reference_text>
            <description>reference.ESA-SP1066</description>
        </External_Reference>
        <External_Reference>
            <reference_text>
                   &apos;Encounters with Comet Halley, The first results&apos;, Nature, Volume 321, No.
                   6067, 15 May 1986.
            </reference_text>
            <description>reference.NATURE321</description>
        </External_Reference>
    </Reference_List>
    
    <Instrument_Host>
        <name>SAKIGAKE</name>
        <type>Spacecraft</type>
        <naif_host_id>SAKIG</naif_host_id>

        <description>
 
    Instrument Host Overview
    ========================
 
      Planet-A and MS-T5 are identical except for their
      scientific payloads.  The main spacecraft body is a
      cylinder, 140 cm in diameter and 70 cm high.  The
      spinning spacecraft is about 250 cm high, from the
      top of the high- gain antenna dish to the bottom of
      the medium-gain antenna.  Its outer wall is covered
      by solar cells which produce 100 W of power under
      optimum conditions.
 
      An equipment platform mounted to a central thrust
      tube carries most of the subsystems, including the
      mechanically despun, high-gain antenna, two
      hydrazine fuel tanks, the thrusters, and the
      experiment sensors.  A star scanner and a nutation
      damper are attached to the thrust tube.  Planet-A
      and MS-TS weigh 139.5 kg and 138.1 kg,
      respectively, including lO kg of hydrazine
      propellant in each case.  Both spacecraft are
      spin-stabilized, with the facility to change the
      spin rate.  The spin axes of both spacecraft will
      be kept perpendicular to the ecliptic plane.  The
      spacecraft/Earth geometry and the data-rate
      requirements preclude the use of a single antenna
      for the duration of the mission.  The antenna
      subsystem therefore consists of a high-gain
      antenna, a medium-gain antenna as a backup, and a
      low-gain antenna for near-Earth operation.  The
      despun high-gain antenna has an offset- parabolic
      reflector with a diameter of 80 cm and a gain of
      21.5 dB in uplink and 22.5 dB in downlink
      transmission.  The communications subsystem
      operates in 5-band using a 5 W transmitter.  MS-T5
      has four data formats(Table below).  The data rates
      of both spacecraft are 2048 bit/s (without coding)
      in &apos;high bit rate&apos; and 64 bit/s (with convolutional
      coding) in &apos;low bit rate&apos; mode.  The bit rate used
      will depend on the communication distance.
 
      The ground station for the mission has been built
      at Usuda, about 170 km northwest of Tokyo.  The
      station&apos;s 64 m diameter dish antenna has a gain of
      approximately 63 dB.  A 64 bit/s communication link
      (convolutionally encoded PCM) is expected to be
      possible from 1.1 AU, which will be the comet-Earth
      distance during the Planet-A encounter.
 
 
 
 
 --------------------------------------------------------------------------
 Table. The MS-T5 scientific payload
 
 
 Experiment  Mass  Power  Data rate         Principal Investigator
             (kg)  (W)    Format 1/2/3/4
 --------------------------------------------------------------------------
                           H 512/768/768/0  H. Oya, Faculty of Science,
 PWP          5.2*  1.7    L 32/48/48/0     Tohoku Univ., Sendai
 
 SOW          2.0   1.1    H 512/768/0/768  K. Oyama, Res. Div. Planetary
                           L 32/48/0/48     Science, ISAS, Tokyo
 
                           H 400/0/768/768  T. Saito, Faculty of Science,
 IMF          5.4** 2.     L 25/0/48/48     Tohoku Univ., Sendai
 --------------------------------------------------------------------------
 Format 1       PWP      SOW      IMF   H = High bit rate
        2       PWP      SOW            L = law bit rate
        3       PWP      IMF
        4       SOW      IMF
 
  * Includes dipole antenna, search coil and electronics
 ** Includes boom
 
 

        </description>
    </Instrument_Host>
</Product_Context>
