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Titlebook: Earth Sciences in the Age of the Satellite; Jean Pouquet Book 1974 D. Reidel Publishing Company, Dordrecht, Holland 1974 energy.formation.

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樓主: 極大
31#
發(fā)表于 2025-3-27 00:12:39 | 只看該作者
32#
發(fā)表于 2025-3-27 02:52:50 | 只看該作者
33#
發(fā)表于 2025-3-27 09:05:57 | 只看該作者
34#
發(fā)表于 2025-3-27 09:59:57 | 只看該作者
From Galileo to Aldrin and Armstrongwas irregular and not smooth. We now know that this observation — and many others of Galileo — was a correct one, but the opposition that always arises against research too far ahead of its time resulted in his condemnation.
35#
發(fā)表于 2025-3-27 14:39:51 | 只看該作者
The Electromagnetic Spectrum. All objects reflect to a greater or lesser extent the radiation emitted by the Sun, or any other source of energy. All objects, provided their temperature is above absolute zero (0 K, ?273°C) emit radiations part of which can be perceived by special instruments.
36#
發(fā)表于 2025-3-27 20:31:46 | 只看該作者
The Visible and Near Infrared of the Electromagnetic Spectrum film register only reflected radiation; the remainder of the solar energy is absorbed by objects, atmospheric gases, and/or refracted by the upper atmospheric boundary and/or diffracted by the atmosphere itself.
37#
發(fā)表于 2025-3-28 00:11:26 | 只看該作者
Broad Principles of Interpretationemitted. Thus, the first aspect to consider is ‘the surface.’ Next we shall deal with the basic principles leading to interpretation of reflected radiations, the main part of the chapter being devoted to emitted daytime and nighttime radiation.
38#
發(fā)表于 2025-3-28 04:23:44 | 只看該作者
39#
發(fā)表于 2025-3-28 08:14:44 | 只看該作者
Wilhelm Weber,Herbert Zogelmannwas irregular and not smooth. We now know that this observation — and many others of Galileo — was a correct one, but the opposition that always arises against research too far ahead of its time resulted in his condemnation.
40#
發(fā)表于 2025-3-28 12:54:02 | 只看該作者
https://doi.org/10.1007/978-3-322-80538-6. All objects reflect to a greater or lesser extent the radiation emitted by the Sun, or any other source of energy. All objects, provided their temperature is above absolute zero (0 K, ?273°C) emit radiations part of which can be perceived by special instruments.
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