Data Set Information
|
DATA_SET_NAME |
GSSR V RTLS 5 12.6-12.9CM RADAR SCALED ECHO POWER/ALT V1.0
|
DATA_SET_ID |
GSSR-V-RTLS-5-12.6-9CM-V1.0
|
NSSDC_DATA_SET_ID |
XD-B2A
|
DATA_SET_TERSE_DESCRIPTION |
This archive contains Venus altimetry images derived from data
acquired by the Goldstone Solar System Radar.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
The Goldstone Solar System Radar observations of Venus from
1972 until 1988 are included in this data set. The system
operated at 12.6 cm up until 1977; afterward the system
operated at 12.9 cm. The data consist of radar scaled
backscatter cross sections in image format and, in most cases,
associated altimetry observations. The data were acquired over
52 separate observing runs. In total the observations cover
the region between approximately 260 degrees (leftmost) east
longitude to 30 degrees (rightmost) east longitude, within
approximately 20 degrees of the equator. Backscatter data were
acquired with opposite sense circular polarization with
incidence angles typically less than 10 degrees. Associated
altimetric data were acquired using a two or three station
interferometric system. Data are presented in Mercator
projection with degrees/pixel in longitude dependent on the
individual data file.
Processing Level Id : 5
Software Flag : N
Processing Start Time : 1972-06-01
Processing Stop Time : 1990-04-01
Parameters
==========
Data Set Parameter 'RADAR SCALED BACKSCATTER CROSS SECTION'
-----------------------------------------------------------
Cross section values that are scaled by some procedure, such
as dividing by theoretical or empirical scattering laws.
Data Set Parameter Name : RADAR SCALED BACKSCATTER
CROSS SECTION
Data Set Parameter Unit : DIMENSIONLESS
Sampling Parameter Name : PIXEL
Sampling Parameter Unit : N/A
Minimum Sampling Parameter : N/A
Maximum Sampling Parameter : N/A
Sampling Parameter Resolution : N/A
Sampling Parameter Interval : N/A
Minimum Available Sampling Int : N/A
Noise Level : UNK
Source Instrument Parameters
============================
Instrument Host ID : GSSR
Data Set Parameter Name : RADAR SCALED BACKSCATTER
CROSS SECTION
Instrument Parameter Name : RADAR ECHO POWER
Important Instrument Parameters : 1
Measurement Information
=======================
Atmospheric Conditions
----------------------
NOT APPLICABLE
Source
------
The transmitter was the 64 meter antenna at the Goldstone
Deep Space Network station.
Calibration Standard
--------------------
NOT APPLICABLE
Wavelength Calibration
----------------------
The transmitter frequency is calibrated with a hydrogen
maser.
Processing
==========
N/A
|
DATA_SET_RELEASE_DATE |
1990-06-15T00:00:00.000Z
|
START_TIME |
1972-06-20T12:00:00.000Z
|
STOP_TIME |
1988-07-27T12:00:00.000Z
|
MISSION_NAME |
PRE-MAGELLAN
|
MISSION_START_DATE |
1968-11-09T12:00:00.000Z
|
MISSION_STOP_DATE |
1988-07-27T12:00:00.000Z
|
TARGET_NAME |
VENUS
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
GSSR
|
INSTRUMENT_NAME |
RADIO TELESCOPE
|
INSTRUMENT_ID |
RTLS
|
INSTRUMENT_TYPE |
RADAR
|
NODE_NAME |
Geosciences
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Overview
========
Pre-1977 backscatter images are normalized relative to the
square root of the scattering properties for an annulus about
the sub-Earth point including the data. The 1977 and later
images are normalized relative to the average scattering
properties for the annulus. Most of the backscatter images are
speckle noise limited as opposed to thermal noise. The
confidence is usually limited by the number of looks. The
errors in the altimetry data are difficult to estimate and vary
greatly over the image. These errors depend upon the accuracy
of the ephemeris, the variation of the interferometer fringe
spacings, the signal to noise ratio and therefore the
scattering law appropriate for each day's observation. The
maximum likelihood estimator also does not provide an estimate
of the errors. Errors range from 30 meters near the sub-radar
region to a few kilometers at the outer edge of the image.
|
CITATION_DESCRIPTION |
Jurgens, R. F., GSSR V RTLS 5 12.6-12.9CM RADAR SCALED ECHO
POWER/ALT V1.0, GSSR-V-RTLS-5-12.6-9CM-V1.0, NASA Planetary Data
System, 1990
|
ABSTRACT_TEXT |
The Goldstone Solar System Radar observations of Venus from 1972
until 1988 are included in this data set. The system operated at
12.6 cm up until 1977 operated at 12.9 cm. The data consist of
radar scaled backscatter cross sections in image format and, in
most cases, associated altimetry observations. The data were
acquired over 52 separate observing runs. In total the
observations cover the region between approximately 260 degrees
(leftmost) east longitude to 30 degrees (rightmost) east
longitude, within approximately 20 degrees of the equator.
Backscatter data were acquired with opposite sense circular
polarization with incidence angles typically less than 10
degrees. Associated altimetric data were acquired using a two or
three station interferometric system. Data are presented in
Mercator projection with degrees/pixel in longitude dependent on
the individual data file.
|
PRODUCER_FULL_NAME |
RAYMOND F. JURGENS
|
SEARCH/ACCESS DATA |
Geosciences Web Services
Geosciences Online Archives
|