Data Set Information
|
DATA_SET_NAME |
LRO MOON LASER ALTIMETER 5 SHADR V1.0
|
DATA_SET_ID |
LRO-L-LOLA-5-SHADR-V1.0
|
NSSDC_DATA_SET_ID |
|
DATA_SET_TERSE_DESCRIPTION |
Spherical harmonic topographic (shape)
and gravity potential models from the
2009 Lunar Reconnaissance Orbiter (LRO)
mission.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
Topographic spherical harmonic coefficients are derived from gridded
altimetry products via a numerical transform. The data are in the form
of tables with a detached label. The Reduced Data Record Software
Interface Specification describes the values input to the harmonic
transform.
The discrete-Fourier-transformed topography coefficients H_j(m) at
latitude index, times the associated Legendre polynomial P_lm, times a
weight proportional to the area associated with a given latitude interval,
are summed over all latitudes to yield the complex coefficient
(C_lm,S_lm). The weights are normalized so that a coefficient of unit
magnitude represents a harmonic whose squared amplitude integrated with
respect to area over a unit sphere is 4 pi.
|
DATA_SET_RELEASE_DATE |
2011-03-15T00:00:00.000Z
|
START_TIME |
2009-07-03T12:00:00.000Z
|
STOP_TIME |
2011-08-10T04:36:55.073Z
|
MISSION_NAME |
LUNAR RECONNAISSANCE ORBITER
|
MISSION_START_DATE |
2009-06-18T12:00:00.000Z
|
MISSION_STOP_DATE |
N/A (ongoing)
|
TARGET_NAME |
MOON
|
TARGET_TYPE |
SATELLITE
|
INSTRUMENT_HOST_ID |
LRO
|
INSTRUMENT_NAME |
LUNAR ORBITER LASER ALTIMETER
|
INSTRUMENT_ID |
LOLA
|
INSTRUMENT_TYPE |
LASER ALTIMETER
|
NODE_NAME |
Geosciences
|
ARCHIVE_STATUS |
|
CONFIDENCE_LEVEL_NOTE |
Overview
========
Data are edited and selected before averaging so as to maintain
good quality. Where necessary, crossover analysis is done prior to
averaging so as to minimize discrepancies between individual tracks.
Data Coverage and Quality
=========================
Each nominal monthly orbit provides roughly two tracks per degree of
longitude at the equator. After each month's data are accumulated,
crossover adjustments are made to minimize the difference in elevation
between closely registered tracks and to remove along- and across-track
orbital errors. The resulting dataset provides better geodetic control
than that from individual tracks. The first release (March 15, 2010)
does not incorporate these adjustments, and relies on preliminary
trajectory solutions. Re-release with better precision and increased
density will occur periodically.
The current release does not include a gravity potential model.
Limitations
===========
Density of observations increases linearly with time. Higher-resolution
SHADR products will be provided when data density provides coverage in a
majority of pixels of each data product.
|
CITATION_DESCRIPTION |
Neumann, G.A., 2009, Lunar Orbiter Laser
Altimeter Spherical Harmonic Model,
LRO-L-LOLA-5-SHADR-V1.0,
NASA Planetary Data System,
2009.
|
ABSTRACT_TEXT |
This data set contains spherical harmonic topographic (shape)
and gravity potential models from the Lunar Orbiter Laser Altimeter
instrument, LRO Laser Ranging, and radio tracking.
|
PRODUCER_FULL_NAME |
GREGORY A. NEUMANN
|
SEARCH/ACCESS DATA |
Geosciences Web Service
Geosciences Online Archives
Lunar Orbital Data Explorer
|