The power spectrum of the seeing during solar observations

Details The power spectrum of the seeing during solar observations The power spectrum of the seeing during solar observations

Publishing date

2011-12-02

URL

arxiv.org/abs/1112.0401v1

Science

Astronomy and Astrophysics

Field

Astrophysics

SubField

Solar and Stellar Astrophysics

Additional info

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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