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Titlebook: Observational Astrophysics; Pierre Léna Textbook Apr 20141st edition Springer-Verlag Berlin Heidelberg 1988 astrophysics.atmosphere.develo

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书目名称Observational Astrophysics
编辑Pierre Léna
视频video
丛书名称Astronomy and Astrophysics Library
图书封面Titlebook: Observational Astrophysics;  Pierre Léna Textbook Apr 20141st edition Springer-Verlag Berlin Heidelberg 1988 astrophysics.atmosphere.develo
描述For the last twenty years astronomy has been developing dramatically. Until the nineteen-fifties, telescopes, spectrometers, and photographic plates consti­ tuted a relatively simple set of tools which had been refined to a high degree of perfection by the joint efforts of physicists and astronomers. Indeed these tools helped at the birth of modern astrophysics: the discovery of the expan­ sion of the Universe. Then came radioastronomy and the advent of electronics; the last thirty years have seen the application to astrophysics of a wealth of new experimental techniques, based on the most advanced fields of physics, and a constant interchange of ideas between physicists and astronomers. Last, but not least, modern computers have sharply reduced the burden of dealing with the information painfully extracted from the skies, whether from ever­ scarce photons, or from the gigantic data flows provided by satellites and large telescopes. The aim of this book is not to give an extensive overview of all the tech­ niques currently in use in astronomy, nor to provide detailed instructions for preparing or carrying out an astronomical project. Its purpose is methodologi­ cal: photons are sti
出版日期Textbook Apr 20141st edition
关键词astrophysics; atmosphere; development; information; photometry; physics; spectra
版次1
doihttps://doi.org/10.1007/978-3-662-02554-3
issn_series 0941-7834
copyrightSpringer-Verlag Berlin Heidelberg 1988
The information of publication is updating

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,The Earth’s Atmosphere,the volatile elements because of its mobility; it separated the sublunar world from that of the stars. Between the time of Galileo and the conquest of space, it limited observable photons to the narrow visible window, radio frequencies being added only latterly..
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Spectral Analysis,by astrophysicists. The examples are legion: energy balance, abundances of molecules, atoms, ions or other particles, macroscopic or microscopic velocity fields, local physical conditions such as the temperature, the density, the magnetic or electric fields, states of equilibrium or of deviation from equipartition of energy ...
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Images,An observer only perceives the three dimensions of space projected on the celestial sphere. The received intensity is the integral of the energy locally emitted into the .. Decoding the measured information to deduce the local conditions is an . which is always delicate.
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