Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jqsrt..40..221j&link_type=abstract
Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 40, Sept. 1988, p. 221-238.
Astronomy and Astrophysics
Astronomy
16
Astronomical Spectroscopy, Infrared Astronomy, Laser Spectroscopy, Molecular Spectra, Planetary Atmospheres, Fourier Transformation, Laser Modes, Semiconductor Diodes, Spectral Line Width, Tunable Lasers
Scientific paper
Infrared spectroscopy of planetary atmospheres is performed at high spectral resolution comparable to that in the laboratory. This requires that laboratory spectroscopy use the highest resolution and the most accurate techniques. Tunable diode laser spectroscopy can supply many of the spectroscopic parameters needed by astronomers. In particular, line positions, line strengths, and collisional line widths are measured with diode lasers, and these are often among the best values available. Diode laser spectra are complimentary to lower resolution, broader-coverage Fourier transform spectra. Certain procedures must be adopted, however, when using diode lasers, for determining their output characteristics and for calibrating each spectrum against quality references.
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