Titlebook: Atomic and Molecular Radiative Processes; With Applications to Vladimir Krainov,Boris M. Smirnov Book 2019 Springer Nature Switzerland AG 2

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Book 2019atoms. Lastly, topical examples in atmospheric and climate change science are presented, such as lightning channel glowing, emission of the solar photosphere, and the greenhouse phenomenon in the atmospheres of the Earth and Venus. . Along with researchers, both graduate and undergraduate students i

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Photon Interaction with Clusters and Microparticles,tal particle. In particular, from the analysis of experimental data it is shown that light absorption is described by radiative transitions in individual atoms which interact strongly with surrounding ones. In addition, electrons of the metal particles screen an electromagnetic field, and if a parti

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Greenhouse Effect in Atmospheres of Earth and Venus,follows from the NASA measurements. The contribution to this temperature change due to injections of carbon dioxide in the atmosphere due to combustion of fossil fuel, and it is 0.02 K. The infrared radiative flux to the Venus surface due to . is about 30% of the total flux, and the other part is de

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1615-5653 uch as lightning channel glowing, emission of the solar photosphere, and the greenhouse phenomenon in the atmospheres of the Earth and Venus. . Along with researchers, both graduate and undergraduate students i978-3-030-21957-4978-3-030-21955-0Series ISSN 1615-5653 Series E-ISSN 2197-6791

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Springer Series on Atomic, Optical, and Plasma Physicshttp://image.papertrans.cn/b/image/164786.jpg

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a system of electrons located in the Coulomb motionless center, we have that bound atomic states has a discrete character and bound energy states are described by certain quantum numbers. A weakness of interaction between an atom and radiation field follows from a small velocity of bound electrons c

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as the impact and quasistatic theories of broadening of spectral lines. Criteria for various mechanisms of line broadening are given and combined cases are considered. Properties of an equilibrium radiation field for a strong interaction with an atomic system are given, and laws of blackbody radiat

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