Ultraviolet radiation on the surface of Mars and the Beagle 2 UV sensor

By Manish R. Patel, J. Zarnecki, David C. Catling. 2002

134 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/c92045d85f109cdf5490daa1a4173cd4da97a171

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In Astronomy and Astrophysics

1. P. Mathe
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Citations in the corpus

• Amino acid photostability on the Martian surface (2005, methodology): “If this intensity is compared to the predicted noontime equatorial insolation at Mars’ surface in a low atmospheric-dust scenario (Patel et al. 2002), then the deuterium lamp provides ∼4% of the UV experienced on Mars in the range of 190 nm to 325 nm.”
• Mineralogy and evolution of the surface of Mars: A review (2007, background): “The martian atmosphere evidences a complex photochemistry, resulting from the intense UV radiation (Patel et al., 2002), and producing strongly oxidising species that react with the regolith (Oyama and Berdahl, 1979).”