Aims. Daily observation conditions are needed when observing the Sun at high angular resolution. MISOLFA is a daytime seeing monitor developed for this purpose that allows the estimation of the spatial and temporal parameters of atmospheric turbulence. This information is necessary, for instance, for astrometric measurements of the solar radius performed at Calern 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 is less sensitive to vibrations and guiding defaults of the telescope since it uses short-exposure images. It is based on the comparison o...
International audiencePICARD is a space mission developed mainly to study the geometry of the Sun. T...
International audiencePICARD is a space mission developed to observe the Sun at high angular resolut...
L'objectif est de comprendre d'effet de la turbulence optique sur la mesure au sol du rayon solaire....
Aims. Daily observation conditions are needed when observing the Sun at high angular resolution. MIS...
International audiencePICARD is a space mission launched in June 2010 to study mainly the geometry o...
International audienceGround based solar observations are strongly affected by optical turbulence. T...
International audienceThe statistical analysis of angle-of-arrival fluctuations appears to be well a...
International audienceDeveloped at the Observatoire de la Côte d'Azur (OCA) within the framework of ...
International audienceThe Franco-Algerian Monitor of Solar Images (MISOLFA) was developped in order ...
The objective is to understand the effect of optical turbulence on ground-based solar radius measure...
International audienceThe statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be...
International audiencePICARD is a space mission developed mainly to study the geometry of the Sun. T...
International audiencePICARD is a space mission developed to observe the Sun at high angular resolut...
L'objectif est de comprendre d'effet de la turbulence optique sur la mesure au sol du rayon solaire....
Aims. Daily observation conditions are needed when observing the Sun at high angular resolution. MIS...
International audiencePICARD is a space mission launched in June 2010 to study mainly the geometry o...
International audienceGround based solar observations are strongly affected by optical turbulence. T...
International audienceThe statistical analysis of angle-of-arrival fluctuations appears to be well a...
International audienceDeveloped at the Observatoire de la Côte d'Azur (OCA) within the framework of ...
International audienceThe Franco-Algerian Monitor of Solar Images (MISOLFA) was developped in order ...
The objective is to understand the effect of optical turbulence on ground-based solar radius measure...
International audienceThe statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be...
International audiencePICARD is a space mission developed mainly to study the geometry of the Sun. T...
International audiencePICARD is a space mission developed to observe the Sun at high angular resolut...
L'objectif est de comprendre d'effet de la turbulence optique sur la mesure au sol du rayon solaire....