By R. M. Goody, Y. L. Yung
A whole revision of Goody's vintage 1964 paintings, this quantity deals a scientific dialogue of atmospheric radiation approaches that this day are on the middle of globally examine and problem. It offers with the ways that incident sunlight radiation is reworked into scattered and thermal radiation, and the thermodynamic outcomes for the Earth's gaseous envelope, selecting features of the interplay among radiation and atmospheric motions because the critical topic for atmospheric radiation reviews. As an entire therapy of actual and mathematical foundations, the textual content assumes no past wisdom of atmospheric physics. The theoretical dialogue is systematic, and will as a result be utilized with minor extension to any planetary surroundings.
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Extra info for Atmospheric Radiation: Theoretical Basis
Keeling, C. , and Whorf, T. , 1985, "Seasonal amplitude increase in the atmospheric CO2 concentration at Mauna Loa, Hawaii, 19591982," J. Geophys. Res. 90, 10529. Isotopic ratios are given by Evans, R. , 1955, The atomic nucleus. New York: McGraw-Hill. Data on atmospheric aerosol and clouds are reviewed by Mason, B. , 1957, The physics of clouds. Oxford: The Clarendon Press. Junge, C. , and Manson, J. , 1961, "Stratospheric aerosol studies," /. Geophys. Res. 66, 2163. Pruppacher, H. , and Klett, J.
The equations that we have used are readily generalized if we allow for the fact that u may now be either the upper or the lower level for a u+*k transition. 65) we may write a balance equation, A similar equation can be written for the lower level, /. To solve these equations we require the collisional coefficients b(u, k). 82), the incident radiation Iv must include solar radiation where solar absorption can cause transitions between coupled levels or species. Both of the foregoing equations are written in the form appropriate to u>k.
1. Introduction For the rest of this chapter, we shall be concerned with formal mathematical manipulation of the equation of transfer needed for subsequent chapters. No new physics is introduced and the reader may treat the remaining paragraphs of this chapter as appendixes, to be consulted when the equations are required. There are, of course, physical grounds for choosing the particular models treated. 4 the model of a plane-parallel atmosphere is introduced, first for an isotropic thermal source function with uniform isotropic boundary conditions, and second for a scattering source function with a nearly parallel incident flux as an upper boundary condition.
Atmospheric Radiation: Theoretical Basis by R. M. Goody, Y. L. Yung