Three-dimensional semi-empirical climate model of water vapor distribution and its implementation to the radiation module of the middle and upper atmosphere model


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Abstract

To provide the more accurate simulation of stationary planetary waves and atmospheric tides using the middle and upper atmosphere model (MUAM), the three-dimensional (longitude-latitude-height) semi-empirical climate model of water vapor distribution in the troposphere was developed which takes into account seasonal variations. The modules of radiation heating and cooling in the MUAM model were modified taking into account the dependence of water vapor concentration on longitude. The simulations performed using the modified version of MUAM revealed that the consideration of water vapor concentration variability along the circle of latitude leads to the substantial dependence of solar heating on longitude that affects the amplitudes of stationary planetary waves in the stratosphere.

About the authors

T. S. Ermakova

Russian State Hydrometeorological University

Author for correspondence.
Email: taalika@mail.ru
Russian Federation, Malookhtinskii pr. 98, St. Petersburg, 195196

I. A. Statnaya

Russian State Hydrometeorological University

Email: taalika@mail.ru
Russian Federation, Malookhtinskii pr. 98, St. Petersburg, 195196

I. N. Fedulina

Almaty University of Power Engineering and Telecommunications

Email: taalika@mail.ru
Kazakhstan, ul. Baitursynova 126, Almaty, 050013

E. V. Suvorova

Russian State Hydrometeorological University

Email: taalika@mail.ru
Russian Federation, Malookhtinskii pr. 98, St. Petersburg, 195196

A. I. Pogoreltsev

Russian State Hydrometeorological University

Email: taalika@mail.ru
Russian Federation, Malookhtinskii pr. 98, St. Petersburg, 195196


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