The power spectrum of the seeing during solar observations

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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5 pages, 5 figures, proc. of 12th Italian-Korean Symposium on Relativistic Astrophysics, July 4-8, 2011, Pescara, Italy

Type

Scientific paper

Abstract

Measurements of the power spectrum of the atmospheric seeing in the line of
sight of the Sun, in the range 0.001-1 Hz, have been performed in Santa Maria
degli Angeli Lucernaria Dome, at IRSOL and in Huairou Station. This study is
aimed to understand the criticity of the meridian transits method for solar
diameter monitoring.

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