Paper
30 November 2017 Dynamics of the refractive properties of the atmosphere at the Big solar vacuum telescope site: new calculating method
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Proceedings Volume 10466, 23rd International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 104660T (2017) https://doi.org/10.1117/12.2284307
Event: XXIII International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2017, Irkutsk, Russian Federation
Abstract
The dynamics of turbulent characteristics including air index refraction vertical variations as well as effective turbulent velocity important for the functioning of the Large solar vacuum telescope (LSVT) adaptive optics system is considered. Long-term changes of the effective turbulent velocity and Fried radius in the atmospheric layer from 0 to 20 km are estimated using model of turbulence taking into account the shape of the energy spectrum over a wide range of spatial and temporal scales. The possible experimental local model of Fried radius changes is discussed for the Large solar vacuum telescope site.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. Yu. Shihovtsev, P. G. Kovadlo, V. P. Lukin, and A. V. Kiselev "Dynamics of the refractive properties of the atmosphere at the Big solar vacuum telescope site: new calculating method", Proc. SPIE 10466, 23rd International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 104660T (30 November 2017); https://doi.org/10.1117/12.2284307
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KEYWORDS
Turbulence

Atmospheric optics

Telescopes

Atmospheric modeling

Optical turbulence

Atmospheric physics

Refractive index

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