Modelling of the propagation of passive impurities in Sevastopol bays

We discuss the results of numerical experiments modelling the process of propagation of passive impurities from the Karantinnaya Bay caused by steady wind currents and turbulent diffusion. The currents are computed according to the Felzenbaum model for the cases of northeast and north-west winds [1, 2]. We analyse specific features of the space and time distribution of the impurities caused by the three-dimensional character of the currents. Translated by Peter V. Malyshev and Dmitry V. Malyshev     

Simulation of the Seasonal Variability of Hydrothermodynamical Fields in Lake Kinneret

We discuss the results of a numerical experiment devoted to the investigation of the variability of the three-dimensional fields of temperature and current velocity brought about by the seasonal variability of external factors: solar radiation, atmospheric fields, discharge of the river Jordan, and water intake for economic necessities. We use a multilayer model in isopycnic coordinates with an upper mixed layer. We set atmospheric factors in the form of monthly average fields that are uniform over space and linearly interpolated in time. We compare the computed fields of heat flux and evaporation through the lake surface, level, temperature, and currents with data of observations. We note a qualitative agreement of temperature fields during the whole year and current velocities in winter when the lake is, in fact, barotropic. In summer when the lake is stratified, currents in the model turn out to be weaker than in observations.     

Emission lines of the red-dwarf flare star EV Lac: Stellar flares

We present equivalent widths and profiles for H_α H_β, H_γ and He I λ4471 Å emission lines obtained in observations of the flares of EV Lac made at the Crimean Astrophysical Observatory in 1994 and 1995. Our semi-empirical modeling of the flares gives insight into the structure of the emitting regions, including a temperature plateau, and also into the physical parameters, size, and location of the star’s relatively quiescent chromosphere.     

Theory of the isotropic scattering of radiation in a plane layer: Feasibility of obtaining a complete analytical solution of the problem

Analytical investigations of the method of linear nonsingular integral equations, originally proposed by É. Kh. Danielyan [Astrofizika 36,225 (1993)] for the solution of problems in the theory of radiative transport in a medium of finite optical thickness with isotropic scattering, are continued in the present article. It is shown that the solution of problems of the stated class reduce to the determination of only the functions u ^± (, ) in the general case with true absorption. Explicit expressions are obtained for these functions at =0. The feasibility of a complete analytical solution of the problem is newly formulated as the solution of a Fredholm integral equation on the semiaxis with a kernel that admits representation by a superposition of exponential functions [Eq. (25)]. The choice of an efficient procedure for determining the Ambartsumyan -function for a semiinfinite medium is discussed. In particular, a new equation is given for this function.Translated from Astrofizika, Vol. 37, No. 1, pp. 129–145, January–March, 1994.