The Ultraviolet Spectrometer investigation on the Pioneer Venus Orbiter mission was extremely successful. The instrument was designed, built and tested at CU/LASP and delivered on time and within budget. The spacecraft and its instruments were required to operate for 243 days in Venus orbit. OUVS operated successfully for a further 13 years with only minor problems. The major scientific results listed above that deal with Venus were all unexpected and significant discoveries. The Comet Halley observations came about because of a favorable alignment of Halley, the Sun, and Venus, and were an important contribution to the international study of this comet. The scientific results of the OUVS investigation are to be found in the 41 papers liste...
The science objectives of Pioneer Venus and future investigations of the planet are discussed. Conce...
Analysis and interpretation of data from the Orbiter Retarding Potential Analyzer (ORPA) onboard the...
The opportunity to determine the planetwide temperature and cloud structure of Venus using radio occ...
The Pioneer Venus Orbiter has been in operation since orbit insertion on December 4, 1978. For the p...
In the present reporting period we have met with the Pioneer Venus PI to collaborate on the recalibr...
The work performed during the 12-month period of this contract involved: (1) further analysis of lat...
The celescope instrumentation and data analysis system is described, the major problems encountered ...
An orbiter and a multiprobe spacecraft will be sent to Venus in 1978 to conduct a detailed examinati...
The three observing programs under NASA Grant NAG5-1913 are described. They are NSOSS, VEOEB, and PC...
Issued as Quarterly progress reports, nos. 2,6,8,9, Semiannual status reports, nos. [1],3,4, Annual ...
The plans to scan Halley's Comet at close range using the Pioneer Venus Orbiter are discussed. The c...
Identical ultraviolet photometer experiments were carried on the eccentric orbiting OGO-5 spacecraft...
The 1976/77 multiple probe mission of the Pioneer Venus spacecraft is discussed, along with the 1978...
In order to characterize possible variations in the abundance and distribution of subcloud sulfuric ...
The 200-inch Hale telescope has been used to obtain high-resolution maps, on four mornings juxtapose...
The science objectives of Pioneer Venus and future investigations of the planet are discussed. Conce...
Analysis and interpretation of data from the Orbiter Retarding Potential Analyzer (ORPA) onboard the...
The opportunity to determine the planetwide temperature and cloud structure of Venus using radio occ...
The Pioneer Venus Orbiter has been in operation since orbit insertion on December 4, 1978. For the p...
In the present reporting period we have met with the Pioneer Venus PI to collaborate on the recalibr...
The work performed during the 12-month period of this contract involved: (1) further analysis of lat...
The celescope instrumentation and data analysis system is described, the major problems encountered ...
An orbiter and a multiprobe spacecraft will be sent to Venus in 1978 to conduct a detailed examinati...
The three observing programs under NASA Grant NAG5-1913 are described. They are NSOSS, VEOEB, and PC...
Issued as Quarterly progress reports, nos. 2,6,8,9, Semiannual status reports, nos. [1],3,4, Annual ...
The plans to scan Halley's Comet at close range using the Pioneer Venus Orbiter are discussed. The c...
Identical ultraviolet photometer experiments were carried on the eccentric orbiting OGO-5 spacecraft...
The 1976/77 multiple probe mission of the Pioneer Venus spacecraft is discussed, along with the 1978...
In order to characterize possible variations in the abundance and distribution of subcloud sulfuric ...
The 200-inch Hale telescope has been used to obtain high-resolution maps, on four mornings juxtapose...
The science objectives of Pioneer Venus and future investigations of the planet are discussed. Conce...
Analysis and interpretation of data from the Orbiter Retarding Potential Analyzer (ORPA) onboard the...
The opportunity to determine the planetwide temperature and cloud structure of Venus using radio occ...