Data Set Information
|
DATA_SET_NAME |
120-COLOR LUNAR NIR SPECTROPHOTOMETRY DATA V1.0
|
DATA_SET_ID |
MK88-L-120CVF-3-RDR-120COLOR-V1.0
|
NSSDC_DATA_SET_ID |
NULL
|
DATA_SET_TERSE_DESCRIPTION |
This archive contains lunar spectra measured with the McCord
120-COLOR CVF NIR photometer on the Mauna Kea 88-inch telescope.
|
DATA_SET_DESCRIPTION |
This dataset consists of reflectance spectra of small lunar areas
measured in 120 spectral channels from 0.62 to 2.6 micrometers using
the McCord circular-variable-filter (CVF) near-infrared photometer. A
small aperture allows light from the selected lunar area to pass
through the CVF and onto the detector. Each spectral channel is
obtained sequentially as the CVF is rotated. Data were acquired using
the 2.2 m telescope on Mauna Kea, Hawaii. All spectra have been scaled
to a given wavelength. Spectral resolution varies somewhat from run
to run. The first half of the CVF produces data at approximately twice
the spectral resolution as the second half; data points where the two
sections of the CVF were joined are unreliable. All data were acquired
as relative reflectance spectra and were calibrated to scaled
reflectance data using a directional-hemispheric (diffuse) spectrum of
Apollo 16 soil acquired by J. B. Adams. See McCord et al., 1981
[MCCORDETAL1981] and Pieters, 1986 [PIETERS1986] for more detail on
the instrument and calibration procedures.
Data files are named according to the scheme Hknnnn. H stands
for Hawaii. The k represents the original archive tape on which
the data were stored, and is related to the year of observation,
as follows:
8 - 1978
9 - 1978
A - 1980
B - 1981
C - 1981
D - 1982
E - 1983.
The last four digits are the sequential number of the file on the
original archive tape.
|
DATA_SET_RELEASE_DATE |
1998-08-01T00:00:00.000Z
|
START_TIME |
1978-01-01T12:00:00.000Z
|
STOP_TIME |
1983-01-01T12:00:00.000Z
|
MISSION_NAME |
|
MISSION_START_DATE |
|
MISSION_STOP_DATE |
|
TARGET_NAME |
MOON
|
TARGET_TYPE |
SATELLITE
|
INSTRUMENT_HOST_ID |
MK88
|
INSTRUMENT_NAME |
120-COLOR CIRCULAR-VARIABLE-FILTER (CVF) PHOTOMETER
|
INSTRUMENT_ID |
120CVF
|
INSTRUMENT_TYPE |
PHOTOMETER
|
NODE_NAME |
Geosciences
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Acquisition of the 120 data points takes a few minutes; thus, a
120-point spectrum can be affected by the accuracy of guiding on the
Moon as well as changing sky conditions and instrument stability. In
most cases, several independent runs of data taken in sequence were
averaged. Error bars are the standard deviation of this average and
only refer to the repeatability of the measurement under these
conditions.
|
CITATION_DESCRIPTION |
Pieters, C., 120-COLOR LUNAR NIR SPECTROPHOTOMETRY DATA V1.0,
MK88-L-120CVF-3-RDR-120COLOR-V1.0, NASA Planetary Data System,
1998
|
ABSTRACT_TEXT |
This dataset consists of reflectance spectra of small lunar areas
measured in 120 spectral channels from 0.62 to 2.6 micrometers
using the McCord circular-variable-filter (CVF) near-infrared
photometer. A small aperture allows light from the selected lunar
area to pass through the CVF and onto the detector. Each spectral
channel is obtained sequentially as the CVF is rotated. Data were
acquired using the 2.2 m telescope on Mauna Kea, Hawaii. All
spectra have been scaled to a given wavelength. Spectral
resolution varies somewhat from run to run. The first half of the
CVF produces data at approximately twice the spectral resolution
as the second half joined are unreliable. All data were acquired
as relative reflectance spectra and were calibrated to scaled
reflectance data using a directional-hemispheric (diffuse)
spectrum of Apollo 16 soil acquired by J. B. Adams.
|
PRODUCER_FULL_NAME |
CARLE M. PIETERS
|
SEARCH/ACCESS DATA |
Geosciences Web Services
Geosciences Online Archives
|