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