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arXiv · 1112.6187

Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements

Costantino Sigismondi·Andrea Raponi·Giulia De Rosi·Michele Bianda·Renzo Ramelli·Massimo Caccia·Matteo Maspero·Loretta Negrini·Xiaofan Wang
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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.

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Costantino Sigismondi, Andrea Raponi, Giulia De Rosi, Michele Bianda, Renzo Ramelli, Massimo Caccia, Matteo Maspero, Loretta Negrini, Xiaofan Wang. 2011-12-28. Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements. https://doi.org/10.1051/eas%2F1255054

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