Planetary submillimeter spectroscopy

Details Planetary submillimeter spectroscopy Planetary submillimeter spectroscopy

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986plas.rept...39k&link_type=abstract

In NASA, Washington Reports of Planetary Astronomy, 1985 p 39 (SEE N87-12407 03-89)

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Cometary Atmospheres, Molecular Spectra, Planetary Atmospheres, Ammonia, Halley'S Comet, Submillimeter Waves, Uranus (Planet), Water Vapor

Scientific paper

A comprehensive observational strategy was developed for the detection and measurement of molecular lines in the millimeter and submillimeter spectra of planetary atmospheres and comets. A sound observational strategy and the associated analytical capability to begin observations from the Caltech Submm Observatory (CSO) on Mauna Kea in FY 87-88. Comet Halley was observed from the NASA-KAO with the dual-frequency (0.8 and 1.6 mm) receiver and conducted a search for NH3 with the DSN 64 m antenna.

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