Add to ORKGConcurrent objectives involve dynamical information: maintenance of Mars ephemeris accuracy, Mercury closure-point ranging for relativity theory testing, and refinement of spin-vector estimates for Venus and Mercury. This task has been renamed to reflect accurately the research it supports. The backlog of unprocessed Venus data has been sharply reduced; most images from the 1980 to 1982 conjunctions, and half of those from 1986, are essentially finished. Suitably formatted data have been distributed to (non-JPL) scientific collaborators for geologic analysis, and to the Magellan project
Semicontrolled image mosaics of Venus, based on Magellan data, are being compiled at 1:50,000,000, 1...
Maps of Venus based on Magellan data are being compiled at 1:50,000,000, 1:5,000,000 and 1:1,500,000...
A rather broad survey is reported of the Venus radar orbiter possibilities within the period 1983-19...
The primary objective of the Goldstone Solar System Radar is the investigation of solar system bodie...
This task provides for the planning, experiment design, and coordination of the data acquisition and...
The ephemerides needed to acquire radar data at Arecibo from observations of various solar-system ob...
The radar astronomy activities supported by the Deep Space Network are reported. The high power S- a...
The acquisition, processing, and interpretation of radar from Mars are reported with emphasis on the...
The high powered 12.6 cm wavelength radar on the 1000 ft Arecibo reflector is used for a variety of ...
A study of the solar system by means of ground based radar is presented. Emphasis was on developing ...
Radar astronomy is the study of the surfaces and near surfaces of Solar System objects using active ...
This is a brief summary of the science findings of the Magellan mission, principally based on data f...
Design criteria and technology requirements for a system of radar reference devices to be fixed to t...
Disk average brightness temperatures of Mercury were obtained using a 4.6 m radio telescopes. The da...
A catalog of lunar and radar anomalies was generated to provide a base for comparison with Venusian ...
Semicontrolled image mosaics of Venus, based on Magellan data, are being compiled at 1:50,000,000, 1...
Maps of Venus based on Magellan data are being compiled at 1:50,000,000, 1:5,000,000 and 1:1,500,000...
A rather broad survey is reported of the Venus radar orbiter possibilities within the period 1983-19...
The primary objective of the Goldstone Solar System Radar is the investigation of solar system bodie...
This task provides for the planning, experiment design, and coordination of the data acquisition and...
The ephemerides needed to acquire radar data at Arecibo from observations of various solar-system ob...
The radar astronomy activities supported by the Deep Space Network are reported. The high power S- a...
The acquisition, processing, and interpretation of radar from Mars are reported with emphasis on the...
The high powered 12.6 cm wavelength radar on the 1000 ft Arecibo reflector is used for a variety of ...
A study of the solar system by means of ground based radar is presented. Emphasis was on developing ...
Radar astronomy is the study of the surfaces and near surfaces of Solar System objects using active ...
This is a brief summary of the science findings of the Magellan mission, principally based on data f...
Design criteria and technology requirements for a system of radar reference devices to be fixed to t...
Disk average brightness temperatures of Mercury were obtained using a 4.6 m radio telescopes. The da...
A catalog of lunar and radar anomalies was generated to provide a base for comparison with Venusian ...
Semicontrolled image mosaics of Venus, based on Magellan data, are being compiled at 1:50,000,000, 1...
Maps of Venus based on Magellan data are being compiled at 1:50,000,000, 1:5,000,000 and 1:1,500,000...
A rather broad survey is reported of the Venus radar orbiter possibilities within the period 1983-19...