Titlebook: Giant Planets of Our Solar System; Atmospheres, Composi Patrick G. J. Irwin Book 2009Latest edition Springer-Verlag Berlin Heidelberg 2009

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Radiative transfer processes in outer planetary atmospheres,rom specific flyby and orbiting spacecraft missions. There are two main components of the observed spectra that provide atmospheric information: reflected sunlight from the cloud and haze layers, and thermal emission from the atmosphere itself.

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https://doi.org/10.1007/978-3-476-05388-6ng”. As the universe expanded and cooled, numerous particle physics processes and particle-antiparticle annihilations occurred (e.g., Krane, 1996). After about . = 6 s, the universe consisted of some number . protons, . electrons, 0.16. neutrons, 10.. photons, and 10.. neutrinos, all at a temperatur

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