The photochemistry of Titan's mildly reducing N-2 atmosphere is reviewed in terms of general chemical and physical principles. On Titan, mass loss of hydrogen ensures photochemical evolution of methane into less saturated hydrocarbons.
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Univ London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, EnglandUniv London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, England
Cui, J.
Galand, M.
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Univ London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, EnglandUniv London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, England
Galand, M.
Yelle, R. V.
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Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USAUniv London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, England
Yelle, R. V.
Wahlund, J. -E.
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Swedish Inst Space Phys, SE-75121 Uppsala, SwedenUniv London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, England
Wahlund, J. -E.
Agren, K.
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Swedish Inst Space Phys, SE-75121 Uppsala, SwedenUniv London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, England
Agren, K.
Waite, J. H., Jr.
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SW Res Inst, San Antonio, TX 78228 USAUniv London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, England
Waite, J. H., Jr.
Dougherty, M. K.
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Univ London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, EnglandUniv London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, Dept Phys, London SW7 2BW, England