Data Set Information
|
DATA_SET_NAME |
NEAR NLR LEVEL 3 DATA PRODUCTS V1.0
|
DATA_SET_ID |
NEAR-A-NLR-6-EROS-MAPS-MODELS-V1.0
|
NSSDC_DATA_SET_ID |
1996-008A-5
|
DATA_SET_TERSE_DESCRIPTION |
NLR Level 3 Data Products includes spherical harmonic shape and
gravity models, and gridded maps or images of those models.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
The NEAR Laser Rangefinder (NLR) Level 3 Data Products includes
spherical harmonic shape and gravity models, and gridded maps
or images of those models.
Parameters
==========
Spherical harmonic models are tables of coefficients GM, Cmn,
and Smn. ASCII data type (SHA) formats are defined. Each file
contains 2 tables: a header table containing general
parameters for the model (gravitational constant, its
uncertainty, degree and order of the field, normalization
state, reference longitude, and reference latitude) and a
coefficients table (degree m, order n, coefficients Cmn and
Smn, and their uncertainties).
Gridded Digital Map files are image representations
of shape and other parameters. Gravity and topographic values
may be displayed using this data type. Data are formatted
as PDS image objects.
Processing
==========
The Level 2 NLR profiles in the 200 by 200 km orbital phases and
lower are the source of the NLR shape models. Where two ground
tracks intersect, the residual is calculated by linear
interpolation between adjacent shots. The crossover residuals are
used as a measure of data quality and can be used to remove
systematic errors in spacecraft ephemeris and pointing. Crossover
corrections are implemented in two stages via the software described
in [NEUMANNETAL2001], as modified for NLR. The first stage adjusts
for long-wavelength errors due to mis-modeled ephemeris and pointing,
at a period of four cycles per asteroid revolution.
The second stage adjusts higher-frequency errors at a period of ~5
minutes, primarily due to residual pointing mismodeling. Adjustments
are iterated until the crossover residual root-mean-square error is
less than 10 m.
The adjusted profiles are merged by binning observations within a
given grid cell, uniformly spaced in longitude and latitude. The
median value and the number of observations in each bin comprise the
gridded data product.
The gravity field coefficients were obtained by solving systems
of equations with thousands of unknowns. Radio tracking data
in long arcs delimited by propulsive maneuvers, occultations,
etc. were used in solutions that were obtained iteratively
and by least squares.
Data
====
Data are stored on CD-WO volumes. A CD volume was created
for delivery of data to PDS.
ASCII spherical harmonic models are stored in the /LEVEL3/SHA
directory with file names of the form NLRknnnv.SHA, where nnn
is a 3-character modifier specified by the data producer, v is a
version identifier, and k is replaced by G for gravity field or
T for topography/shape field, and SHA denotes that this is an ASCII
file of spherical harmonic coefficients.
Gridded map products are stored in the /LEVEL3/IMG directory.
Each image is a binary array of 16-bit integers with one image line
per file record. The image file name is in the form NLRnnnvk.IMG,
where nnn is the bin size, v is a version identifier, and k is
replaced by C for counts or R for radius, and IMG denotes that
this is a PDS image object. For example, a one-eighth degree
resolution topography image would be named NLR125vR.IMG. Its format
would be described by a detached PDS label in the file NLR125vR.LBL.
An ASCII tabular file containing global shape data of Eros,
including the latitude and longitude of the NLR laser bounce
point, the radius, and the number of observations (counts) can be
found in the /LEVEL3/ASCII directory.
Ancillary Data
==============
None.
Coordinate System
=================
NLR data files use an EROS centered body-fixed coordinate
system with positive east longitude. The transformation from
inertial (J2000) coordinates to body-fixed is represented by the
project-supplied SPICE format attitude and orientation files used
to generate level 2 data products.
Software
========
None.
Media/Format
============
The archival data set was written on CD-WO by the NEAR/NLR
Project. The CD-WO volumes conform to ISO 9660 Level 2
standards.
|
DATA_SET_RELEASE_DATE |
2001-07-13T00:00:00.000Z
|
START_TIME |
2000-03-05T12:00:04.000Z
|
STOP_TIME |
2001-02-12T07:04:01.000Z
|
MISSION_NAME |
NEAR EARTH ASTEROID RENDEZVOUS
|
MISSION_START_DATE |
1996-02-17T12:00:00.000Z
|
MISSION_STOP_DATE |
2001-02-28T12:00:00.000Z
|
TARGET_NAME |
EROS
|
TARGET_TYPE |
ASTEROID
|
INSTRUMENT_HOST_ID |
NEAR
|
INSTRUMENT_NAME |
NEAR LASER RANGEFINDER
|
INSTRUMENT_ID |
NLR
|
INSTRUMENT_TYPE |
ALTIMETER
|
NODE_NAME |
Small Bodies
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Overview
========
Data in this archive have been reduced as part of mission data
analysis activities of the NEAR/NLR Science Team.
Review
======
This archival data set was reviewed by the NEAR/NLR Science
Team prior to final submission to the Planetary Data
System (PDS).
Prior to creation of the final version of the archival data
set, key elements of the archive were distributed for
preliminary review. These included electronic versions of
example PDS labels, example data files, CATALOG files, and other
relevant documentation. These materials were distributed to
PDS personnel, the experiment investigator, and others, as
appropriate.
Data Coverage and Quality
=========================
These volumes contain gravity and shape models and gridded maps
generated from NEAR data collected through February 2001.
The NEAR data included tracking results from the EROS Orbit
Phase.
GTM0180A.SHA contains the coefficients for a 180x180
degree and order shape model produced at Goddard Space Flight
Center. A full error analysis is included.
Internal consistency, as measured by crossover point misfit,
is generally better than 10 m.
NLRG016A.SHA is a spherical harmonic gravity field model
complete to degree and order 16.
NLR125AR.IMG is a gridded shape map of Eros at a
resolution of 0.125 by 0.125 degrees, based on altimetry data
acquired by the NLR instrument. The data include edited NLR
observations from 200-km orbits and lower, using the NLR393
orbit solutions produced at NASA-GSFC.
NLR125AC.IMG is a data file that accompanies the shape
map of Eros NLR125AR.IMG at a resolution of
0.125 by 0.125 degrees. It contains the number of observations
per pixel that have been used to produce the NLR shape data
product. The data include edited NLR observations from 200-km
orbits and lower.
NLR100.TAB is a 1 degree resolution tabular data file that
contains global shape data of Eros, including the latitude and
longitude of the NLR laser bounce point, the radius, and the
number of observations (counts).
Limitations
===========
There is NO gravity covariance matrix on these volumes.
This product is useful in understanding the errors in the gravity
solution. The gravity field covariance represents the complete
error description for the gravity field solution, including the
coefficient variances (sigmas^2), and the correlations between
all the coefficients.
This product was not available at the time this archive was
completed. The file and documentation will be available at a
later date on the World Wide Web/Internet at the following URL:
http://pds-geophys.wustl.edu/pds/near_nlr.
|
CITATION_DESCRIPTION |
Neumann G., D. Smith, NEAR NLR LEVEL 3 DATA PRODUCTS V1.0,
NEAR-A-NLR-6-EROS-MAPS-MODELS-V1.0, NASA Planetary Data System,
2001.
|
ABSTRACT_TEXT |
NLR Level 3 Data Products includes spherical harmonic shape and
gravity models, and gridded maps or images of those models.
|
PRODUCER_FULL_NAME |
DAVID E. SMITH
|
SEARCH/ACCESS DATA |
SBN PSI WEBSITE
Geosciences Web Services
Geosciences Online Archives
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