Effect of atmospheric extinction on solar radial velocity measurements

Details Effect of atmospheric extinction on solar radial velocity measurements Effect of atmospheric extinction on solar radial velocity measurements

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..177b&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 177-179 (SEE N89-25819 19-92)

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Astronomical Photometry, Atmospheric Attenuation, Radial Velocity, Solar Oscillations, Solar Rotation, Velocity Measurement, Ground Stations, Solar Observatories, Solar Spectra, Space Observations (From Earth), Sunlight

Scientific paper

Effects of differential extinction across the Earth's atmosphere on astronomical photometry are reviewed. Under the same circumstances when a rotating extended object is observed spectrometrically, a residual radial velocity is obtained which varies during the day. In the case of integral sunlight observations, this effect was calculated along the day in all possible observing situations during the year. Applications to real observations are shown and discussed leading to conclusions specially relevant to ground-based networks.

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