Probing solar system objects at infrared wavelengths

Details Probing solar system objects at infrared wavelengths Probing solar system objects at infrared wavelengths

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989infph..29..167m&link_type=abstract

(Eidgenoessische Technische Hochschule Zuerich, International Conference on Infrared Physics, 4th, Zurich, Switzerland, Aug. 22-

Astronomy and Astrophysics

Astronomy

2

Infrared Astronomy, Infrared Photometry, Solar System, Spectrum Analysis, Halley'S Comet, Jupiter Atmosphere, Thermal Emission, Water Vapor

Scientific paper

The instruments, techniques, and analysis methods employed in IR observations of solar-system objects are discussed and illustrated with sample data. Particular attention is given to (1) high-resolution (Doppler-limited) spectra of H2O in Comet Halley and Comet Wilson (1986l), obtained with the NASA Kuiper Airborne Observatory in 1985-1986, and (2) scanning observations of Jovian thermal emission, obtained with the NASA IRTF in 1987 and subjected to detailed time-series analysis to investigate atmospheric motion. The data are presented in spectra, energy-level diagrams, maps, and graphs and briefly characterized.

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