Share Email Print
cover

Proceedings Paper • new

Dynamics of the refractive properties of the atmosphere at the Big solar vacuum telescope site: new calculating method
Author(s): A. Yu. Shihovtsev; P. G. Kovadlo; V. P. Lukin; A. V. Kiselev
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper 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.

Paper Details

Date Published: 30 November 2017
PDF: 5 pages
Proc. SPIE 10466, 23rd International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 104660T (30 November 2017); doi: 10.1117/12.2284307
Show Author Affiliations
A. Yu. Shihovtsev, Institute of Solar-Terrestrial Physics (Russian Federation)
V.E. Zuev Institute of Atmospheric Optics (Russian Federation)
P. G. Kovadlo, Institute of Solar-Terrestrial Physics (Russian Federation)
V. P. Lukin, V.E. Zuev Institute of Atmospheric Optics (Russian Federation)
A. V. Kiselev, Institute of Solar-Terrestrial Physics (Russian Federation)


Published in SPIE Proceedings Vol. 10466:
23rd International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics
Oleg A. Romanovskii, Editor(s)

© SPIE. Terms of Use
Back to Top