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Titlebook: Remote Sensing of Atmosphere and Ocean from Space: Models, Instruments and Techniques; Frank S. Marzano,Guido Visconti Book 2002 Springer

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31#
發(fā)表于 2025-3-27 00:54:00 | 只看該作者
32#
發(fā)表于 2025-3-27 04:38:04 | 只看該作者
33#
發(fā)表于 2025-3-27 06:34:15 | 只看該作者
G. P. Gobbi,F. Barnabay it was possible to illustrate the effect of deposition conditions, geometry of the system and kinetic parameters of deposition processes. Besides, three main problems of current density distribution in electrometallurgy were treated semiquantitatively. The edge effect in metal electrorefinning and
34#
發(fā)表于 2025-3-27 10:35:03 | 只看該作者
P. Bauery it was possible to illustrate the effect of deposition conditions, geometry of the system and kinetic parameters of deposition processes. Besides, three main problems of current density distribution in electrometallurgy were treated semiquantitatively. The edge effect in metal electrorefinning and
35#
發(fā)表于 2025-3-27 14:51:11 | 只看該作者
E D R. Westwaterto this important change is the advance of surface spectroscopic techniques able to characterize the complex surfaces of the heterogeneous catalytic system. The Advanced Study Institute (on which the current proceedings is based) has as its primary aim the bringing together of a variety of lecturers
36#
發(fā)表于 2025-3-27 20:16:55 | 只看該作者
37#
發(fā)表于 2025-3-28 00:13:58 | 只看該作者
38#
發(fā)表于 2025-3-28 05:17:51 | 只看該作者
Stephen J. Englishtanding of the mechanisms underlying the development of microstructure in metals during ion irradiation. The earliest investigations were for the bcc metal molybdenum. Since then extensive studies have been made of the structural nature of the gas bubble superlattice in copper. In this metal, and th
39#
發(fā)表于 2025-3-28 08:32:50 | 只看該作者
40#
發(fā)表于 2025-3-28 14:03:50 | 只看該作者
Laurence Eymard temperature have been studied with TEM. At implantation temperatures below about 300°C, Kr precipitation is driven by stochastic (non-diffusional) processes, and the precipitate size-distribution is monomodal. Precipitates with radii less than about 30? are solid Kr while larger precipitates are in
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