Planetary submillimeter spectroscopy

Details Planetary submillimeter spectroscopy Planetary submillimeter spectroscopy

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988plas.rept...75k&link_type=abstract

In NASA, Washington, Reports of Planetary Astronomy, p 75 (SEE N89-16624 08-89)

Physics

Astronomical Spectroscopy, Comets, Deep Space Network, Jupiter (Planet), Solar Physics, Solar Wind, Submillimeter Waves, Uranus (Planet), Ions, Magnetospheres, Venus (Planet)

Scientific paper

The aim is to develop a comprehensive observational and analytical program to study solar system physics and meterology by measuring molecular lines in the millimeter and submillimeter spectra of planets and comets. A primary objective is to conduct observations with new JPL and Caltech submillimeter receivers at the Caltech Submillimeter Observatory (CSO) on Mauna Kea, Hawaii. A secondary objective is to continue to monitor the time variable planetary phenomena (e.g., Jupiter and Uranus) at centimeter wavelength using the NASA antennas of the Deep Space Network (DSN).

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