Bundle Information
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IDENTIFIER |
urn:nasa:pds:kaguya_grs_spectra::1.1
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NAME |
Kaguya Gamma-Ray Spectrometer Corrected Spectra Bundle
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TYPE |
Archive
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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.
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.
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.
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.
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.
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.
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SEARCH/ACCESS DATA |
Kaguya Gamma-Ray Spectrometer Corrected Spectra Online
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Citation |
DIGITAL OBJECT IDENTIFIER (DOI) |
10.17189/1517635
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AUTHOR LIST |
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EDITOR LIST |
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PUBLICATION YEAR |
2019
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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.
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.
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.
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.
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.
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.
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Context |
START DATE TIME |
2007-12-14T04:15:35.000Z
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STOP DATE TIME |
2009-05-28T07:43:22.000Z
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LOCAL MEAN SOLAR TIME |
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LOCAL TRUE SOLAR TIME |
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SOLAR LONGITUDE |
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PRIMARY RESULT PURPOSE |
SCIENCE
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PRIMARY RESULT PROCESSING LEVEL |
Derived
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PRIMARY RESULT DESCRIPTION |
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PRIMARY RESULT WAVELENGTH RANGE |
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PRIMARY RESULT DOMAIN |
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PRIMARY RESULT DISCIPLINE NAME |
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INVESTIGATION |
KAGUYA
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OBSERVING SYSTEM |
Kaguya
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OBSERVING SYSTEM COMPONENT |
Kaguya
GRS
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TARGET |
MOON
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REFERENCES |
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Collections |
DATA COLLECTION |
Kaguya Gamma-Ray Spectrometer Corrected Spectra Collection
Kaguya Gamma-Ray Spectrometer Ephemerides, Pointing and Geometry Collection
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DOCUMENT COLLECTION |
Kaguya Gamma-Ray Spectrometer Corrected Spectra Document Collection
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CONTEXT COLLECTION |
Kaguya Gamma-Ray Spectrometer Context Product Collection
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