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- W4233206473 abstract "Publisher SummaryThe simplest conceivable atmosphere is gravitationally bound (and therefore in hydrostatic equilibrium) and spherically symmetric. This chapter highlights vertical structure of an atmosphere. The vertical structure of an atmosphere is the run of pressure, temperature, density, and chemical composition with distance from the center of the planet. When these parameters are inferred in part from theory or when they are tabulated as mean or representative values, they constitute a model atmosphere. The tropospheric temperature is governed by radiative and convective exchange. The vertical distribution of pressure, temperature, and density in a static, spherical atmosphere with a specified composition are largely governed by three relationships—namely, (1) hydrostatic equilibrium, (2) radiative equilibrium, and (3) convection in the troposphere. The radiative-convective model with a gray atmosphere reproduces the main features of the troposphere temperature distribution, with the radiative “skin temperature” being identified with the near-isothermal region of the tropopause. The departure from grayness itself diminishes the coupling between the ground and skin temperatures. With windows in the absorption spectrum, the ground can cool by radiating directly to space or to the stratosphere." @default.
- W4233206473 created "2022-05-12" @default.
- W4233206473 date "1987-01-01" @default.
- W4233206473 modified "2023-09-27" @default.
- W4233206473 title "Chapter 1 Vertical Structure of an Atmosphere" @default.
- W4233206473 doi "https://doi.org/10.1016/s0074-6142(08)62754-0" @default.
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