Costantino Sigismondi, Andrea Raponi, Xiaofan Wang, Giulia De Rosi, Michele Bianda, Renzo Ramelli
Published 2011-12-02Version 1
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.
Comments: 5 pages, 5 figures, proc. of 12th Italian-Korean Symposium on Relativistic Astrophysics, July 4-8, 2011, Pescara, Italy
Forty two years counting spots: solar observations by D. E. Hadden during 1890-1931 revisited
Modelling the Autocovariance of the Power Spectrum of a Solar-Type Oscillator
Power spectrum of turbulent convection in the solar photosphere
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