DocumentCode :
3448055
Title :
Photovoltaic performance in the Venus environment
Author :
Landis, Geoffrey A. ; Vo, Thomas
Author_Institution :
NASA John Glenn Res. Center, Cleveland, OH, USA
fYear :
2009
fDate :
7-12 June 2009
Abstract :
The harsh environment of Venus makes it a challenging location to use photovoltaics. The difficulties include low solar intensity due to clouds and atmospheric scattering, altered solar spectrum, high operating temperatures, and a corrosive acid environment Incorporating the effect of the Venus atmosphere and clouds on the intensity and spectrum of light available and the effect of the ambient temperature, the efficiency of solar cells is calculated as a function of altitude above the surface. Remarkably, even at the high-temperature conditions of the Venus surface, some performance remains.
Keywords :
Venus; photovoltaic power systems; Venus environment; ambient temperature; atmospheric scattering; corrosive acid environment; high operating temperatures; light available; low solar intensity; photovoltaic performance; solar spectrum; Atmosphere; Clouds; Earth; Light scattering; Photovoltaic cells; Photovoltaic systems; Rayleigh scattering; Solar power generation; Temperature sensors; Venus;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Photovoltaic Specialists Conference (PVSC), 2009 34th IEEE
Conference_Location :
Philadelphia, PA
ISSN :
0160-8371
Print_ISBN :
978-1-4244-2949-3
Electronic_ISBN :
0160-8371
Type :
conf
DOI :
10.1109/PVSC.2009.5411663
Filename :
5411663
Link To Document :
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