Context. To evaluate site quality and to develop multi-conjugative adaptive optics systems for future large solar telescopes, characterization of contributions to seeing from heights up to at least 12 km above the telescope is needed. Aims. We describe a method for evaluating contributions to seeing from different layers along the line-of-sight to the Sun. The method is based on Shack Hartmann wavefront sensor data recorded over a large field-of-view with solar granulation and uses only measurements of differential image displacements from individual exposures, such that the measurements are not degraded by residual tip-tilt errors. Methods. The covariance of differential image displacements at variable field angles provides a natural exten...
International audienceFor a solar adaptive optics system equipped with a Shack-Hartmann wavefront se...
International audienceThe statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be...
International audienceDaily observation conditions are needed when observing the Sun at high angular...
When observing from the ground one has to deal with the turbulence from the atmosphere and the turbu...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
We discuss the use of measurements of the solar granulation contrast as a measure of optical quality...
Day-time turbulence profiles are important for the next generation of Solar Telescopes, which will b...
The European Solar Telescope is a 4-m planned facility designed to have high spatial resolution capa...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
Abstract Adaptive optics (AO), which provides diffraction limited imaging over a field-of-view (FOV)...
Solar diameter measurements performed from ground by several instruments during these last decades s...
Despite the fact that selecting good solar observatory sites is an important matter, day-time seeing...
International audienceIn this work we study in details the influence of pure astronomical refraction...
The National Solar Observatory at Sacramento Peak is developing adaptive optics (AO) for solar astro...
International audienceFor a solar adaptive optics system equipped with a Shack-Hartmann wavefront se...
International audienceThe statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be...
International audienceDaily observation conditions are needed when observing the Sun at high angular...
When observing from the ground one has to deal with the turbulence from the atmosphere and the turbu...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
We discuss the use of measurements of the solar granulation contrast as a measure of optical quality...
Day-time turbulence profiles are important for the next generation of Solar Telescopes, which will b...
The European Solar Telescope is a 4-m planned facility designed to have high spatial resolution capa...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
Abstract Adaptive optics (AO), which provides diffraction limited imaging over a field-of-view (FOV)...
Solar diameter measurements performed from ground by several instruments during these last decades s...
Despite the fact that selecting good solar observatory sites is an important matter, day-time seeing...
International audienceIn this work we study in details the influence of pure astronomical refraction...
The National Solar Observatory at Sacramento Peak is developing adaptive optics (AO) for solar astro...
International audienceFor a solar adaptive optics system equipped with a Shack-Hartmann wavefront se...
International audienceThe statistical analysis of angle-of-arrival ($AA$) fluctuations appears to be...
International audienceDaily observation conditions are needed when observing the Sun at high angular...