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Merge pull request #174 from NASA-PDS-Incubator/i173
Fix bug introduced from #149 fix
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src/test/resources/github173/invalid/bundle_kaguya_derived.xml
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<?xml version="1.0" encoding="UTF-8"?> | ||
<?xml-model href="https://pds.nasa.gov/pds4/pds/v1/PDS4_PDS_1B00.sch" schematypens="http://purl.oclc.org/dsdl/schematron"?> | ||
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<Product_Bundle 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_1B00.xsd"> | ||
<Identification_Area> | ||
<logical_identifier>urn:nasa:pds:kaguya_grs_spectra</logical_identifier> | ||
<version_id>1.1</version_id> | ||
<title>Kaguya Gamma-Ray Spectrometer Corrected Spectra Bundle</title> | ||
<information_model_version>1.11.0.0</information_model_version> | ||
<product_class>Product_Bundle</product_class> | ||
<Citation_Information> | ||
<publication_year>2019</publication_year> | ||
<description> | ||
This archive contains Kaguya Gamma-Ray Spectrometer (KGRS) corrected and calibrated time-series | ||
spectra and ephemerides, pointing, and geometry (EPG) data for the nominal and extended observation | ||
periods of JAXA's SELENE (Kaguya) mission. | ||
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The SELENE mission was the Japanese mission to the Moon with a main orbiter “Kaguya” and | ||
two daughter relay satellites launched on Sep. 14, 2007. KGRS was mounted on the deck of the | ||
main orbiter. It employed a high-purity Ge (HPGe) crystal as a main detector, and surrounding | ||
BGO and plastic scintillators as anti-coincidence detectors to reduce backgrounds. The | ||
Ge crystal was cooled by a Sterling refrigerator. It made close-proximity observations of the | ||
Moon from Dec. 14, 2007 to Dec. 11, 2008 at the high circular orbital altitude of 100 km, and | ||
from Feb. 10 to May 28 in 2009 at the low elliptical orbital altitude of ~30 x 50 km. | ||
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KGRS recorded energy spectra of gamma rays in two gain modes simultaneously; high gain (0.1 | ||
to 3 MeV) and low gain (0.1 to 13 MeV), each of which was analyzed by the 13-bit (8192 ch) | ||
analog-to-digital converter (ADC). While the former has a higher spectral resolution over the | ||
energy range of radioactive elements, the latter has better statistics and covers the whole energy | ||
range of major rock-forming elements, including the Fe neutron capture line at 7.6 MeV. The | ||
accumulation time of each spectrum was 17 s. Both modes of spectra are included in this archive. | ||
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The observation epochs of KGRS consists of three regular measurement periods (Period 1 to 3), | ||
background measurements, and the annealing of the Ge crystal. The HPGe detector was annealed | ||
from 16 to 25, December 2008, which improved energy resolution by a factor of two. | ||
Period 1 and 2 lasted two and five months, respectively, with limited spatial or spectral | ||
resolutions. Period 3 lasted ~3.5 months (including dead time) with the best spatial and spectral | ||
resolutions. In addition, spectra from the background measurement when the satellite was flipped | ||
and the detector faced deep space can be analyzed to estimate the background gamma-ray intensity | ||
from the satellite due to the exposure to galactic cosmic rays. | ||
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This archive consists of three spectrum files (each corresponding to one KGRS epoch) and one unified | ||
EPG file. The spectrum files contain a time series of corrected and calibrated pulse height spectra | ||
acquired by KGRS's HPGe detector in the lunar orbit. In the spectrum files, each row contains the | ||
spacecraft clock (sclk) ticks and UTC time corresponding to the end of the accumulation interval | ||
(17 s), with the two sets of the 8192-channel HPGe spectra accumulated. In the EPG file, each row | ||
starts with sclk recorded at the end of the accumulation interval to match spacecraft positions, | ||
pointing, and correction factors with the corrected spectra. Note that the UTC time and ephemeris time | ||
included in the EPG file correspond to the midpoint of the accumulation interval. | ||
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The Kaguya Gamma-Ray Spectrometer Corrected Spectra bundle was created by Naoyuki Yamashita at Planetary | ||
Science Institute, AZ, USA, with the permission of JAXA and the KGRS instrument PI Prof. Nobuyuki Hasebe. | ||
This work was supported by the NASA under Grant No. NNX16AG54G issued through the Planetary Data Archiving, | ||
Restoration, and Tools Program (PDART), Research Opportunities in Space and Earth Sciences (ROSES) 2015. | ||
</description> | ||
</Citation_Information> | ||
<Modification_History> | ||
<Modification_Detail> | ||
<modification_date>2019-09-30</modification_date> | ||
<version_id>1.0</version_id> | ||
<description>Peer reviewed version of Kaguya Gamma-Ray Spectrometer Corrected Spectra PDS4</description> | ||
</Modification_Detail> | ||
</Modification_History> | ||
</Identification_Area> | ||
<Context_Area> | ||
<Time_Coordinates> | ||
<start_date_time>2007-12-14T04:15:35Z</start_date_time> | ||
<stop_date_time>2009-05-28T07:43:22Z</stop_date_time> | ||
</Time_Coordinates> | ||
<Primary_Result_Summary> | ||
<purpose>Science</purpose> | ||
<processing_level>Derived</processing_level> | ||
</Primary_Result_Summary> | ||
<Investigation_Area> | ||
<name>Kaguya</name> | ||
<type>Mission</type> | ||
<Internal_Reference> | ||
<lid_reference>urn:nasa:pds:context:investigation:mission.kaguya</lid_reference> | ||
<reference_type>bundle_to_investigation</reference_type> | ||
</Internal_Reference> | ||
</Investigation_Area> | ||
<Observing_System> | ||
<name>Kaguya</name> | ||
<Observing_System_Component> | ||
<name>Kaguya</name> | ||
<type>Spacecraft</type> | ||
<Internal_Reference> | ||
<lid_reference>urn:nasa:pds:context:instrument_host:spacecraft.kaguya</lid_reference> | ||
<reference_type>is_instrument_host</reference_type> | ||
</Internal_Reference> | ||
</Observing_System_Component> | ||
<Observing_System_Component> | ||
<name>GRS</name> | ||
<type>Instrument</type> | ||
<Internal_Reference> | ||
<lid_reference>urn:nasa:pds:context:instrument:kaguya.grs</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>collection_to_target</reference_type> | ||
</Internal_Reference> | ||
</Target_Identification> | ||
</Context_Area> | ||
<Reference_List> | ||
<Internal_Reference> | ||
<lid_reference>urn:nasa:pds:kaguya_grs_spectra:document:kgrs_calibrated_spectra</lid_reference> | ||
<reference_type>bundle_to_document</reference_type> | ||
</Internal_Reference> | ||
<Internal_Reference> | ||
<lid_reference>urn:nasa:pds:kaguya_grs_spectra:document:kgrs_ephemerides_doc</lid_reference> | ||
<reference_type>bundle_to_document</reference_type> | ||
</Internal_Reference> | ||
</Reference_List> | ||
<Bundle> | ||
<bundle_type>Archive</bundle_type> | ||
</Bundle> | ||
<Bundle_Member_Entry> | ||
<lid_reference>urn:nasa:pds:kaguya_grs_spectra:data_spectra</lid_reference> | ||
<member_status>Primary</member_status> | ||
<reference_type>bundle_has_data_collection</reference_type> | ||
</Bundle_Member_Entry> | ||
</Product_Bundle> |
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