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Atmospheric Radiation
Yu. M. Timofeyev, E. M. Shulgina
St.
Petersburg State University
tim@troll.phys.spbu.ru
On the basis of materials presented by L. P. Bass (Keldysh Institute of Ap‑
plied Mathematics RAS (IAM RAS)); V. P. Budak (Moscow Power-Engineering
Institute (MPEI)); A. A. Cheremisin (Siberian Federal University (SFU));
N. E. Chubarova, S. A. Terpygova (Lomonosov Moscow State University
(MSU)); G. I. Gorchakov, I. A. Gorchkova, S. A. Sitnov and M. A. Sviridenkov
(Obukhov Institute of Atmospheric Physics (IAP RAS)); I. L Karol (Voeikov
Main Geophysical Observatory, MGO); E. N. Kadygrov (Central Aerological
Observatory (CAO)), A. F. Neryshev (Scientific and Production Association “Ty‑
phoon” (Typhoon); V. I. Perevalov, Yu. N. Ponomarev, S. M. Sakerin,
T. K. Sklyadneva and T. B. Zhuravleva (Zuev Institute of Atmospheric Optics SB
RAS (IAO SB RAS)); V. F. Radionov (Arctic and Antarctic Research Institute
(AARI); A. N. Rublev (Russian Research Center “Kurchatov Institute” (Kurcha‑
tov Institute)); A. B. Uspensky (Scientific Research Center for Space Hydrome‑
teorology “Planeta” (Planeta)).
During 2011–2014 the Russian Radiation Commission in cooperation with
interested departments and institutions hold two International Symposiums on
Atmospheric Radiation and Dynamics (ISARD-2011, ISARD-2013). At these
conferences most actual problems of atmospheric physics (radiation transfer and
atmospheric optics, greenhouse gases,
clouds and aerosols, climate changes, re‑
mote measurement methods, new observation data) were discussed. In this re‑
view, 6 directions of studies covering the complete spectrum of investigations in
atmospheric radiation are given.
1. Radiation Transfer
Numerous investigations in this line are devoted to the theoretical study of
the radiative transfer in different mediums and for different measurement geom‑
etries and the development of methods and algorithms for solving the radiation
transfer equation as applied to different problem of atmospheric optics.
Different methods of radiation transfer theory have been intensely developed
by the MPEI team. The substantiation of the radiative transfer equation (RTE)
has been carried out from the standpoint of statistical optics [Budak and Veklen‑
ko, 2011]. The essential difference of the method using in this article is the
application of the L. V. Keldysh matrix Green’s functions. Traditionally, the
approach used here is the Dyson and Bethe-Salpeter equations. Bethe-Salpeter