International audienceThe MISOLFA seeing monitor is developed to analyze spatial and temporal statistical properties of daytime optical turbulence. It is based on Angle-of-Arrival (AA) statistical properties. The MISOLFA optical device measures AA-fluctuations observed as intensity variations in the pupil plane image formed through a thin slit positioned in the instrument focal plane on the solar edge. Numerical simulations are then performed to ensure the system performances. We present here its basic principles and some obtained results
International audiencePICARD is a space mission launched in June 2010 to study mainly the geometry o...
The observation of the Sun at high angular resolution is of great importance in astronomy. In this c...
Context. This work is a part of the development of observational instruments for the study of optic...
International audienceThe MISOLFA seeing monitor is developed to analyze spatial and temporal statis...
International audienceHigh angular resolution observations of the sun are limited by atmospheric tur...
International audienceHigh angular resolution observations of the sun are limited by atmospheric tur...
International audienceAnisoplanatism in Adaptive Optics or Differential Astrometry as in ground-base...
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 audienceThe Franco-Algerian Monitor of Solar Images (MISOLFA) was developped in order ...
International audienceDaily observation conditions are needed when observing the Sun at high angular...
International audienceThe statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be...
International audiencePICARD is a space mission launched in June 2010 to study mainly the geometry o...
The observation of the Sun at high angular resolution is of great importance in astronomy. In this c...
Context. This work is a part of the development of observational instruments for the study of optic...
International audienceThe MISOLFA seeing monitor is developed to analyze spatial and temporal statis...
International audienceHigh angular resolution observations of the sun are limited by atmospheric tur...
International audienceHigh angular resolution observations of the sun are limited by atmospheric tur...
International audienceAnisoplanatism in Adaptive Optics or Differential Astrometry as in ground-base...
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 audienceThe Franco-Algerian Monitor of Solar Images (MISOLFA) was developped in order ...
International audienceDaily observation conditions are needed when observing the Sun at high angular...
International audienceThe statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be...
International audiencePICARD is a space mission launched in June 2010 to study mainly the geometry o...
The observation of the Sun at high angular resolution is of great importance in astronomy. In this c...
Context. This work is a part of the development of observational instruments for the study of optic...