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Synthetic Infrared Spectra

Published online by Cambridge University Press:  03 August 2017

Robert L. Kurucz
Robert L. Kurucz*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, U.S.A.

Abstract

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The Sun is the star we can observe with the highest spectral resolution and signal-to-noise. From studying the infrared spectrum we can learn about the Sun, about stars in general, and about atomic and molecular spectroscopy. We discuss the computer programs for spectrum synthesis, the infrared flux and central intensity atlases of the solar spectrum, and the atomic and molecular line data. Considerable work is still required to improve the observations and to improve the line data.

Keywords

atomic datainfrared: starsline: formationmolecular dataSun: atmosphere
Type
Part 6: The Infrared Spectrum
Information
Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 523 - 531
Copyright
Copyright © Kluwer 1994 

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