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Titlebook: Observatories in Earth Orbit and Beyond; Proceedings of the 1 Y. Kondo Conference proceedings 1990 Springer Science+Business Media Dordrech

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發(fā)表于 2025-3-25 05:46:26 | 只看該作者
22#
發(fā)表于 2025-3-25 09:27:24 | 只看該作者
M. G. Hauser,T. Kelsall,H. Moseley,R. Silverberg,T. L. Murdock,J. C. Mather,G. Smoot,R. Weiss,E. L. esis of signals, images, and other arrays of data. The material presented here addresses the au- dience of engineers, financiers, scientists, and students looking for explanations of wavelets at the undergraduate level. It requires only a working knowledge or memories of a first course in linear alg
23#
發(fā)表于 2025-3-25 15:29:30 | 只看該作者
24#
發(fā)表于 2025-3-25 17:19:29 | 只看該作者
M. A. C. Perrymangnals, images, and other arrays of data. The material presented here addresses the au- dience of engineers, financiers, scientists, and students looking for explanations of wavelets at the undergraduate level. It requires only a working knowledge or memories of a first course in linear algebra and c
25#
發(fā)表于 2025-3-25 23:01:24 | 只看該作者
26#
發(fā)表于 2025-3-26 00:55:51 | 只看該作者
F. Makino scaling functions and wavelets that have helped the authors to understand wavelets and develop intuition about them. The classes of wavelets in the list below seem to us to capture many of the features that are important for applications or have a special signficance for the mathematical theory. So
27#
發(fā)表于 2025-3-26 05:36:39 | 只看該作者
J. B. Holbergesis of signals, images, and other arrays of data. The material presented here addresses the au- dience of engineers, financiers, scientists, and students looking for explanations of wavelets at the undergraduate level. It requires only a working knowledge or memories of a first course in linear alg
28#
發(fā)表于 2025-3-26 10:30:21 | 只看該作者
29#
發(fā)表于 2025-3-26 13:16:30 | 只看該作者
The Hubble Space Telescopeatellite are working very well, with two key exceptions: The line-of-sight pointing is subject to occasional jitter apparently induced by thermal stresses in the solar arrays; this is expected to be overcome. The telescope mirrors are found to contain approximately 0.5 wave rms of spherical aberrati
30#
發(fā)表于 2025-3-26 18:34:17 | 只看該作者
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