Other
Scientific paper
May 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979icar...38..166f&link_type=abstract
Icarus, vol. 38, May 1979, p. 166-179.
Other
16
Aerothermochemistry, Atmospheric Chemistry, Jupiter Atmosphere, Spectroscopic Analysis, Trace Elements, Abundance, Adiabatic Conditions, Graphs (Charts), High Temperature, Temperature Effects, Thermodynamics, Chemical Composition, Condensation, Carbon Monoxide, Thermodynamics, Trace Elements, Jupiter, Atmosphere, Dynamics, Gases, Tin, Lead, Tellurium, Gallium, Germane, Oxide, Sulfides, Nitrides, Compounds, Cadmium, Antimony, Thallium, Arsenic, Bismuth, Hydrogen, Oxygen, Nitrogen, Sulphur, Phosphorus
Scientific paper
The thermochemistry of several hundred compounds of twelve selected trace elements (Ge, Se, Ga, As, Te, Pb, Sn, Cd, Sb, Tl, In, and Bi) has been investigated for solar composition material along a Jupiter adiabat. The results indicate that AsF3, InBr, TlI, and SbS, in addition to CO, PH3, GeH4, AsH3, H2Se, HCl, HF, and H3BO3 proposed by Barshay and Lewis (1978), may be potential chemical tracers of atmospheric dynamics. The reported observation of GeH4 is interpreted on the basis of new calculations as implying rapid vertical transport from levels where the temperature is greater than or equal to 800 K. Upper limits are also set on the abundances of many gaseous compounds of the elements investigated.
Fegley Bruce
Lewis Scott J.
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