High-resolution infrared spectroscopy of planetary atmospheres

Details High-resolution infrared spectroscopy of planetary atmospheres High-resolution infrared spectroscopy of planetary atmospheres

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pasp...95..691t&link_type=abstract

(Astronomical Society of the Pacific, Symposium on the Renaissance in High-Resolution Spectroscopy - New Techniques, New Frontie

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, High Resolution, Infrared Spectroscopy, Planetary Atmospheres, Emission Spectra, Far Infrared Radiation, Fourier Transformation, Optical Heterodyning, Spaceborne Astronomy, Spectral Resolution

Scientific paper

Various techniques for high-resolution infrared spectroscopy of planetary atmospheres are reviewed. Resolving powers of 106 are now possible at 1 - 5 μm with Fourier transform spectrometers and at 10 μm with heterodyne spectrometers. The extension of high-resolution spectroscopy to the far-infrared is currently under development. The role of ground-based high-resolution spectroscopy compared to observations by spacecraft is discussed.

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