Day-time turbulence profiles are important for the next generation of Solar Telescopes, which will be equipped with multi conjugate adaptive optics systems. We measured daytime turbulence profiles above La Palma from 17th to 19th September 2013 using a wide- field wave-front sensor. The measured profiles are consistent with previous measurements and suggest that the majority of the turbulence is located close to the ground. Our method does not yet permit precise measurements of high altitude turbulence due to limited instrument and analysis sensitivity
As telescopes become larger, into the era of ∼40 m Extremely Large Telescopes, the high-resolution v...
The performance of adaptive optics (AO) systems are highly dependent upon optical turbulence. Thus, ...
Atmospheric profiling is a requirement for controlling wide-field Adaptive Optics (AO) instruments, ...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
Context. Space weather has become acutely critical for today’s global communication networks. To und...
Ground based telescopes suffer from degraded resolution due to aberrations induced by the atmosphere...
The European Solar Telescope is a 4-m planned facility designed to have high spatial resolution capa...
Aims. Daily observation conditions are needed when observing the Sun at high angular resolution. MIS...
Local atmospheric turbulence at the telescope level is regarded as a major reason for affecting the ...
A six-night optical turbulence monitoring campaign has been carried at Cerro Paranal observatory in ...
Advanced Adaptive Optics (AO) instruments on ground-based telescopes require accurate knowledge of t...
Atmospheric turbulence has two effects in astronomy; (i) the broadening of the point spread function...
Optical turbulence represented by the structure function parameter of the refractive index Cn2 is re...
Ground-based astronomy suffers from waveform distortion produced by the turbulent atmosphere, which ...
As telescopes become larger, into the era of ∼40 m Extremely Large Telescopes, the high-resolution v...
The performance of adaptive optics (AO) systems are highly dependent upon optical turbulence. Thus, ...
Atmospheric profiling is a requirement for controlling wide-field Adaptive Optics (AO) instruments, ...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
This paper presents preliminary daytime profiles taken using a Wide-Field Shack-Hartmann Sensor at t...
Context. Space weather has become acutely critical for today’s global communication networks. To und...
Ground based telescopes suffer from degraded resolution due to aberrations induced by the atmosphere...
The European Solar Telescope is a 4-m planned facility designed to have high spatial resolution capa...
Aims. Daily observation conditions are needed when observing the Sun at high angular resolution. MIS...
Local atmospheric turbulence at the telescope level is regarded as a major reason for affecting the ...
A six-night optical turbulence monitoring campaign has been carried at Cerro Paranal observatory in ...
Advanced Adaptive Optics (AO) instruments on ground-based telescopes require accurate knowledge of t...
Atmospheric turbulence has two effects in astronomy; (i) the broadening of the point spread function...
Optical turbulence represented by the structure function parameter of the refractive index Cn2 is re...
Ground-based astronomy suffers from waveform distortion produced by the turbulent atmosphere, which ...
As telescopes become larger, into the era of ∼40 m Extremely Large Telescopes, the high-resolution v...
The performance of adaptive optics (AO) systems are highly dependent upon optical turbulence. Thus, ...
Atmospheric profiling is a requirement for controlling wide-field Adaptive Optics (AO) instruments, ...