Add to ORKGAn algorithm is described for constructing the model of the Venus surface as an expansion in spherical functions. The relief expansion coefficients were obtained up to the coefficient S sub 99. The surface picture representation is given according to this expansion. The surface model constructed was used for processing radar observations. The use of the surface model allows improved agreement between the design and measured values of radar ranges
This lithograph shows a mosaic of Venus that was composed from Magellan images taken during radar in...
The VASSIS task was to design and develop an imaging system and container for operation above the su...
Mariner II radar and radiometric observations of Venus during 1962 conjunction - physical dat
The physographic curves of the moon and terrestrial planets, drawn both for the entire surface as a ...
The surface of Venus has remained a relative mystery because of the very dense atmosphere that is op...
The examination of Venus topography, obscured for photographic imaging, is reported in the applicati...
Design criteria and technology requirements for a system of radar reference devices to be fixed to t...
The study deals with materials of radar mapping: Venus surface from Venera-15,16 automatic interplan...
Maps of Venus based on Magellan data are being compiled at 1:50,000,000, 1:5,000,000 and 1:1,500,000...
Magellan's altimeter is providing some of the finest resolution topography of Venus achieved to date...
AbstractSince the Magellan radar mapping of Venus in the early 1990’s, techniques of synthetic apert...
A rather broad survey is reported of the Venus radar orbiter possibilities within the period 1983-19...
Concurrent objectives involve dynamical information: maintenance of Mars ephemeris accuracy, Mercury...
In the late 1970s and early 1980s, the United States and the Soviet Union sent the Pioneer Venus and...
The concept, constraints, and capabilities of a radar altimeter type contour mapper for a Venus orbi...
This lithograph shows a mosaic of Venus that was composed from Magellan images taken during radar in...
The VASSIS task was to design and develop an imaging system and container for operation above the su...
Mariner II radar and radiometric observations of Venus during 1962 conjunction - physical dat
The physographic curves of the moon and terrestrial planets, drawn both for the entire surface as a ...
The surface of Venus has remained a relative mystery because of the very dense atmosphere that is op...
The examination of Venus topography, obscured for photographic imaging, is reported in the applicati...
Design criteria and technology requirements for a system of radar reference devices to be fixed to t...
The study deals with materials of radar mapping: Venus surface from Venera-15,16 automatic interplan...
Maps of Venus based on Magellan data are being compiled at 1:50,000,000, 1:5,000,000 and 1:1,500,000...
Magellan's altimeter is providing some of the finest resolution topography of Venus achieved to date...
AbstractSince the Magellan radar mapping of Venus in the early 1990’s, techniques of synthetic apert...
A rather broad survey is reported of the Venus radar orbiter possibilities within the period 1983-19...
Concurrent objectives involve dynamical information: maintenance of Mars ephemeris accuracy, Mercury...
In the late 1970s and early 1980s, the United States and the Soviet Union sent the Pioneer Venus and...
The concept, constraints, and capabilities of a radar altimeter type contour mapper for a Venus orbi...
This lithograph shows a mosaic of Venus that was composed from Magellan images taken during radar in...
The VASSIS task was to design and develop an imaging system and container for operation above the su...
Mariner II radar and radiometric observations of Venus during 1962 conjunction - physical dat