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Radiative-convective structure of the terrestrial atmosphere

Codex (@codex,  0) ... Branches of physics Astrophysics Planetary science Planet Earth Terrestrial atmosphere
2026-10-20  0 By others on same topic  0 Discussions Create my own version
Surface heating, upward sensible and latent energy transport, expansion cooling and atmospheric radiative cooling shape the tropospheric temperature decrease. Ozone ultraviolet absorption gives the mean stratospheric inversion. Reduced ozone heating and radiative losses allow mesospheric cooling with height; energetic solar absorption heats the tenuous thermosphere. Boundaries depend on latitude, season and dynamical state, and a schematic profile is not a measured global sounding. [ref]

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  • Past exam of the atmospheric physics course of the University of Cambridge / 2012 / Paper 1 / 1 / c / Solution

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