Parametric model of the Earth’s radiation budget     

Zastawny  A. 《Meteorology and Atmospheric Physics》2004,85(4):275-281

Summary Proposition of the Earths radiation budget, based on properties of the absorption, reflection and scattering coefficients, is presented. In the model, the final fluxes of radiation are expressed directly by absorption properties of the atmospheres components. Consequently, total (i.e., with all feedback) greenhouse effect, forced by any component of the atmosphere, can be determined. Presented model is averaged and one dimensional, but it can be developed if it meets with acceptance.  相似文献   

Calculation of solar and thermal radiation absorption in the atmosphere, based on the HITRAN data     

A. Zastawny 《Meteorology and Atmospheric Physics》2006,92(1-2):153-159

Summary Using the HITRAN database from 2003, the absorption of solar and thermal radiation by the atmosphere is calculated. The results are presented in the form of spectral densities of absorption yield of the atmosphere and its components, and fractions of absorbed energy of the solar radiation and thermal radiation in the atmosphere by each of its components separately and together. Finally, the obtained results are discussed in the context of the lately published model of Earth’s radiation budget-MAP 85(4), 275–281 (2004). The shares of atmospheric components in the greenhouse effect and in the absorption of solar radiation are calculated. The percentage contributions of the more important atmospheric components in the greenhouse effect are as follows: clouds 66, water vapor 25, CO₂ 6.7, N₂O 0.7, CH₄ 0.7.  相似文献   

Theoretical model of a magnetic white dwarf     

I. Bednarek  A. Brezina  R. Ma&#x;ka  M. Zastawny‐Kubica 《Astronomische Nachrichten》2003,324(5):425-431

In this paper a theoretical model of a magnetic white dwarf is studied. All numerical calculations are performed under the assumption of a spherically symmetric star. The obtained equation of state is stiffer with the increase of value of the magnetic field (B). Numerical values of the maximum mass and radius are presented. The influence of the magnetic field on the results is evident. Finally the departure from the condition of isothermality of a degenerate electron gas in the gravitational field is discussed.  相似文献