Aims. Daily observation conditions are needed when observing the Sun at high angular resolution. MISOLFA is a daytime seeingmonitor developed for this purpose that allows the estimation of the spatial and temporal parameters of atmospheric turbulence. Thisinformation is necessary, for instance, for astrometric measurements of the solar radius performed at Cale Observatory (France)with SODISM II, the ground-based version of the SODISM instrument of the PICARD mission.Methods. We present a new way to estimate the spatial parameters of atmospheric turbulence for daily observations. This method
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نویسنده: کامران عباسی
تاريخ: جمعه
27 مرداد
1396 ساعت: 14:01