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Titlebook: Chemistry of the Lower Atmosphere; S. I. Rasool (Deputy Director) Book 1973 Plenum Press, New York 1973 atmosphere.biology.chemistry.forma

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發(fā)表于 2025-3-23 13:22:09 | 只看該作者
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發(fā)表于 2025-3-23 17:47:37 | 只看該作者
https://doi.org/10.1007/978-3-319-24510-2ere will be other changes in the future. The question is not whether our climate will change, but rather: What causes it to change? If we knew the answer, perhaps we would be able to foresee the future climates in store for us.
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發(fā)表于 2025-3-23 18:57:31 | 只看該作者
Miscellaneous Quantum Algorithms,activity has perturbed the natural carbon cycle on a global scale. In a sense, this injection is a mammoth geochemical experiment. It permits us to observe the transient response of the air, the oceans, and the biosphere to a major disturbance taking place over the interval of only a few years. Our
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發(fā)表于 2025-3-24 00:29:48 | 只看該作者
Particulate Matter in the Lower Atmosphere,nclude theoretical and experimental physics, meteorology, astronomy, and chemistry. This chapter describes results obtained by such disciplines, discusses in detail many of the aspects of more than average interest, and suggests several problems that remain to be solved.
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發(fā)表于 2025-3-24 03:21:55 | 只看該作者
The Chemical Basis for Climate Change,ere will be other changes in the future. The question is not whether our climate will change, but rather: What causes it to change? If we knew the answer, perhaps we would be able to foresee the future climates in store for us.
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發(fā)表于 2025-3-24 09:49:22 | 只看該作者
https://doi.org/10.1007/978-1-4684-1986-3atmosphere; biology; chemistry; formation; history; ocean; solar system; water
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發(fā)表于 2025-3-24 11:34:56 | 只看該作者
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發(fā)表于 2025-3-24 17:48:42 | 只看該作者
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發(fā)表于 2025-3-24 21:13:18 | 只看該作者
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發(fā)表于 2025-3-25 02:46:54 | 只看該作者
Book 1973, in Exobiology, edited by C. Ponnamperuma, North Holland Publishing Co. ), we tried to describe why we believe that in the early history of the solar system all the terrestrial planets lost the atmospheres of H2 and He which they had acquired from the solar nebula at the time of their formation. Th
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