Data Set Information
|
DATA_SET_NAME |
P12 V RADIO SCIENCE SUBSYSTEM RESAMPLED LOS GRAVITY V1.0
|
DATA_SET_ID |
P12-V-RSS-4-LOS-GRAVITY-V1.0
|
NSSDC_DATA_SET_ID |
XD-B2A
|
DATA_SET_TERSE_DESCRIPTION |
This dataset contains line of sight (LOS) gravity estimates
derived from Pioneer Venus Doppler tracking measurements acquired
during the Pioneer Venus Orbiter mission.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
Line of sight (LOS) gravity data were obtained as part of the
Radio Science Experiment by tracking 351 orbits of the Pioneer
Venus Orbiter. The data set consists of a table with the
following columns: spacecraft latitude, longitude (degrees),
accelerations, and altitude (km). The acceleration data were
determined from differentiation of raw Doppler residuals and
are expressed as units of mm/s**2. To obtain LOS gravity in
milligals, accelerations need to be multiplied by 100. An
acceleration of 1.20 mm/s**2, therefore, corresponds to 120
mgal, a large gravity anomaly.
An accompanying file contains ancillary data to supplement the
gravity data file. The accompanying file has one record for
each orbit in which LOS gravity data were acquired. Each
record contains the minimum and maximum latitude and longitude,
and altitudes for the orbit, along with the sub-earth point
latitude and longitude, and the spacecraft location and
velocity in a Venus centered coordinate system. Each record
also contains a pointer to the first record for that orbit in
the gravity data file, and the number of records for that
orbit.
Processing Level Id : 4
Software Flag : N
Processing Start Time : 1978
Processing Stop Time : 1990
Parameters
==========
Data Set Parameter 'LINE OF SIGHT ACCELERATION'
-----------------------------------------------
The acceleration of the spacecraft due to planet mass
anomalies, where acceleration is measured along the line of
sight between the spacecraft antenna and the Deep Space Net.
Obtained by tracking Doppler changes in telemetry frequency.
Data Set Parameter Name : LINE OF SIGHT ACCELERATION
Data Set Parameter Unit : MM/S**2
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 : P12
Data Set Parameter Name : LINE OF SIGHT ACCELERATION
Instrument Parameter Name : RSSDETEB POWER
Important Instrument Parameters : 1
Processing
==========
N/A
|
DATA_SET_RELEASE_DATE |
1990-06-15T00:00:00.000Z
|
START_TIME |
1978-01-01T12:00:00.000Z
|
STOP_TIME |
1980-01-01T12:00:00.000Z
|
MISSION_NAME |
PIONEER
PRE-MAGELLAN
|
MISSION_START_DATE |
1978-05-20T12:00:00.000Z
1968-11-09T12:00:00.000Z
|
MISSION_STOP_DATE |
1992-10-08T12:00:00.000Z
1988-07-27T12:00:00.000Z
|
TARGET_NAME |
VENUS
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
P12
|
INSTRUMENT_NAME |
RADIO SCIENCE SUBSYSTEM
|
INSTRUMENT_ID |
RSS
|
INSTRUMENT_TYPE |
RADIO SCIENCE
|
NODE_NAME |
Geosciences
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Overview
========
There are several possible sources for error, including the
Earth's troposphere and ionosphere, Venus' atmosphere, and
space plasma. The noise levels were very dynamic and changed
from day to day. For specific information see Sjogren et al.,
1980.
|
CITATION_DESCRIPTION |
Sjogren, W. L., P12 V RADIO SCIENCE SUBSYSTEM RESAMPLED LOS
GRAVITY V1.0, P12-V-RSS-4-LOS-GRAVITY-V1.0, NASA Planetary Data
System, 1990
|
ABSTRACT_TEXT |
Line of sight (LOS) gravity data were obtained as part of the
Radio Science Experiment by tracking 351 orbits of the Pioneer
Venus Orbiter. The data set consists of a table with the
following columns: spacecraft latitude, longitude (degrees),
accelerations, and altitude (km). The acceleration data were
determined from differentiation of raw Doppler residuals and are
expressed as units of mm/s**2. To obtain LOS gravity in
milligals, accelerations need to be multiplied by 100. An
acceleration of 1.20 mm/s**2, therefore, corresponds to 120 mgal,
a large gravity anomaly.
|
PRODUCER_FULL_NAME |
WILLIAM L. SJOGREN
|
SEARCH/ACCESS DATA |
Geosciences Web Services
Geosciences Online Archives
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