You have requested a machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Neither SPIE nor the owners and publishers of the content make, and they explicitly disclaim, any express or implied representations or warranties of any kind, including, without limitation, representations and warranties as to the functionality of the translation feature or the accuracy or completeness of the translations.
Translations are not retained in our system. Your use of this feature and the translations is subject to all use restrictions contained in the Terms and Conditions of Use of the SPIE website.
29 November 2016Some approaches to describe the vertical structure of air refraction index variations
The features of air index refraction vertical variations up to 20 km at the Large solar vacuum telescope site are discussed. The possible local model of air index refraction fluctuations are supposed at the Large solar vacuum telescope site.
The alert did not successfully save. Please try again later.
P. G. Kovadlo, A. Yu. Shikhovtsev, V. P. Lukin, L. A. Bolbasova, "Some approaches to describe the vertical structure of air refraction index variations
," Proc. SPIE 10035, 22nd International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 100351P (29 November 2016); https://doi.org/10.1117/12.2249028