The 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 de- vice measures AA-fluctuations observed as intensity variations in the pupil plane image formed through a thin slit positioned in the...
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June 16, 2003 (v1)Conference paperUploaded on: December 4, 2022
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September 9, 2003 (v1)Conference paper
High angular resolution observations of the sun are limited by atmospheric turbulence. The MISOLFA seeing monitor (still under construction) is developed to obtain spatial and temporal statistical properties of optical turbulence by analyzing local motions observed on solar edge images. The solar flying shadows used for angle-of-arrival...
Uploaded on: December 3, 2022 -
May 28, 2001 (v1)Conference paper
The one dimensional point spread function for long exposure frames of the whole system atmosphere-instrument is deduced from solar limb observations using data recorded at Calern Observatory (France). It is then compared to the theoretical one deduced from the Von Karman model. Good agreement is found allowing to deduce the spatial coherence...
Uploaded on: December 3, 2022 -
September 18, 2001 (v1)Conference paper
The one-dimensional point spread function for long-exposure frames of the whole system atmosphere - instrument is calculated from solar limb observations using data recorded at OCA Observatory (France). It is then compared to the theoretical one deduced from the Von Karman model and various wave-front structure functions. Good agreement is...
Uploaded on: December 3, 2022 -
May 28, 2001 (v1)Conference paper
The statistical analysis of angle-of-arrival fluctuations appears to be well adapted to monitor the optical effects induced by the atmospheric turbulence on the images observed using ground-based telescopes. In daytime, these fluctuations may be easily observed on solar limb images. In the context of the comparison planned between solar...
Uploaded on: December 4, 2022 -
November 13, 2000 (v1)Conference paper
The statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be well adapted to monitor the optical effects induced by the atmospheric turbulence on the images observed using ground-based telescopes. In daytime, these fluctuations may be easily observed on solar limb images. In the context of the comparison planned between solar...
Uploaded on: December 4, 2022