Мақола

Energy Spectra of Atmospheric Turbulence for Calculating Cn2 Parameter. I. Maidanak and Suffa Observatories in Uzbekistan

A. Yu. ShikhovtsevInstitute of Astronomy, Russian Academy of Sciences, 119017 Moscow, RussiaP. G. KovadloInstitute of Solar-Terrestrial Physics, Siberian Branch of the Russian Academy of Sciences, 664033 Irkutsk, RussiaE. A. KopylovInstitute of Astronomy, Russian Academy of Sciences, 119017 Moscow, RussiaM. IbrahimovInstitute of Astronomy, Russian Academy of Sciences, 119017 Moscow, RussiaSh. A. EhgamberdievDepartment of Astronomy and Astrophysics, Physics Faculty, National University of Uzbekistan, Tashkent 100174, UzbekistanYusufjon TillayevDepartment of Astronomy and Astrophysics, Physics Faculty, National University of Uzbekistan, Tashkent 100174, Uzbekistan

Atmospherejournal2021en

ABI

Аннотация

Knowledge of the turbulence spectra is of interest for describing atmospheric conditions as applied to astronomical observations. This article discusses the deformations of the turbulence spectra with heights in a wide range of scales at the sites of the Maidanak and Suffa observatories. It is shown that the energy of baroclinic instability is high at the sites of these observatories and should be taken into account in the calculations of the refractive index structure constant Cn2.

Мавзулар

Solar and Space Plasma Dynamics Adaptive optics and wavefront sensing Geophysics and Gravity Measurements

Идентификаторлар

DOI: 10.3390/atmos12121614

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