A Method for Determination of Water Vapor Content from Solar Spectrum: Preliminary Results

Details A Method for Determination of Water Vapor Content from Solar Spectrum: Preliminary Results A Method for Determination of Water Vapor Content from Solar Spectrum: Preliminary Results

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pobeo..90..141j&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 90, pp. 141-146

Astronomy and Astrophysics

Astronomy

Scientific paper

For precise spectrophotometric observations of solar spectral lines, it is necessary to remove the systematical errors caused by telluric line blending. Calibration methods are usually applied for removing these errors. Calibration in the case of telluric lines that originate from water vapor is more complicated than in the case of molecular oxygen lines, since the amount of water vapor in Earth atmosphere is unpredictable. We present here a method for determination of water vapor amount in atmosphere, based on the measured ratio of water vapor and molecular oxygen spectral line parameters.

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