Other
Scientific paper
Dec 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.241..175r&link_type=abstract
The Atmospheres of Saturn and Titan, Proceedings of an International Workshop held in Alpbach, Austria, 16-19 September, 1985.
Other
1
Planetary Atmospheres:Chemistry, Planetary Atmospheres:Laboratory Simulations
Scientific paper
Particles with kinetic energies exceeding a few eV are relatively frequent in space. They induce chemical reactions different from those considered in cosmic chemistry hitherto and include endothermic reactions with high activation energies and atom-molecule interactions. This "hot atom chemistry" leads to the formation of molecules in rings and icy surfaces as well as in the upper atmosphere of planets and satellites. An important contribution comes from secondary particles generated by cosmic rays in the deeper layers of the atmospheres and the oceans. Laboratory simulation is performed by ion implantation and optical spectroscopy, chemical sputtering and mass spectroscopy, as well as by nuclear recoil techniques and radiochromatography. The variation of the chemical products with the radiation dose gives information on radiation chemistry in space.
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