The power spectrum of the seeing during solar observations
Solar and Stellar Astrophysics
2011-12-05 v1 Atmospheric and Oceanic Physics
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.
Keywords
Cite
@article{arxiv.1112.0401,
title = {The power spectrum of the seeing during solar observations},
author = {Costantino Sigismondi and Andrea Raponi and Xiaofan Wang and Giulia De Rosi and Michele Bianda and Renzo Ramelli},
journal= {arXiv preprint arXiv:1112.0401},
year = {2011}
}
Comments
5 pages, 5 figures, proc. of 12th Italian-Korean Symposium on Relativistic Astrophysics, July 4-8, 2011, Pescara, Italy