Studies of radiative transfer in planetary atmospheres

Details Studies of radiative transfer in planetary atmospheres Studies of radiative transfer in planetary atmospheres

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984umassrept.....i&link_type=abstract

Semiannual Status Report, 1 Jun. - 30 Nov. 1984 Massachusetts Univ., Amherst. Dept. of Physics and Astronomy.

Astronomy and Astrophysics

Astronomy

Atmospheric Composition, Cometary Atmospheres, Planetary Atmospheres, Radiative Transfer, Hydroxyl Emission, Interstellar Matter, Lunar Maria, Molecular Clouds, Porous Materials, Radio Astronomy

Scientific paper

Progress is reported in modeling cometary emission in the 18-cm OH transition with specific application and predictions for Comet Halley. Radiative transfer is also being studied in rough and porous media. The kinematics of the cold, dark interstellar cloud Li34N were examined, and CO monitoring of Venus and Mars continues. Analysis of 3.4 mm maps of the lunar surface shows thermal anomalies associated with such surface features as the Crater Copernicus, Mare Imbrium, Mare Nubium, Mare Serenitatis, and Mare Tranquillatis.

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