Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements [PDF]
Costantino Sigismondi, Andrea Raponi, Giulia De Rosi, Michele Bianda, Renzo Ramelli, Massimo Caccia, Matteo Maspero, Loretta Negrini, Xiaofan WangMeasurements 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.View original: http://arxiv.org/abs/1112.6187
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