Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements
Instrumentation and Methods for Astrophysics
2015-06-03 v1 Solar and Stellar Astrophysics
Abstract
Measurements of the power spectrum of the seeing in the range 0.001-1 Hz have been performed in order to understand the criticity of the transits' method for solar diameter monitoring.
Cite
@article{arxiv.1112.6187,
title = {Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements},
author = {Costantino Sigismondi and Andrea Raponi and Giulia De Rosi and Michele Bianda and Renzo Ramelli and Massimo Caccia and Matteo Maspero and Loretta Negrini and Xiaofan Wang},
journal= {arXiv preprint arXiv:1112.6187},
year = {2015}
}
Comments
3 pages, 3 figures, proc. of the Fourth French-Chinese meeting on Solar Physics Understanding Solar Activity: Advances and Challenges, 15 - 18 November, 2011 Nice, France