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Titlebook: Chaos in Astrophysics; J. R. Buchler,J. M. Perdang,E. A. Spiegel Book 1985 D. Reidel Publishing Company, Dordrecht, Holland 1985 astrophys

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發(fā)表于 2025-3-21 18:35:43 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Chaos in Astrophysics
編輯J. R. Buchler,J. M. Perdang,E. A. Spiegel
視頻videohttp://file.papertrans.cn/224/223880/223880.mp4
叢書(shū)名稱(chēng)Nato Science Series C:
圖書(shū)封面Titlebook: Chaos in Astrophysics;  J. R. Buchler,J. M. Perdang,E. A. Spiegel Book 1985 D. Reidel Publishing Company, Dordrecht, Holland 1985 astrophys
描述The per iod of an oscillator tells us much about its structure. J. J. Thomson‘s deduction that a particle with the e/rn of an electron was in the atom is perhaps the most stunning instance. For us, the deduction of the mean density of a star from its oscillation period is another important example. What then can we deduce about an oscillator that is not periodic? If there are several frequencies or if the behavior is chaotic, may we not hope to learn even more delicate vital statistics about its workings? The recent progress in the theory of dynamical systems, particularly in the elucidat ion of the nature of chaos, makes it seem reasonable to ask this now. This is an account of some of the happenings of a workshop at which this question was raised and discussed. ~iTe were inc0rested in seeing ways in which the present understanding of chaos might guide astrophysical modelling and the interpretation of observations. But we did not try to conceal that we were also interested in chaos itself, and that made for a pleasant rapport between the chaoticists and astrophysicists at the meeting. We have several introductory papers on chaos in these proceedings, particularly on the analysis o
出版日期Book 1985
關(guān)鍵詞astrophysics; star; turbulence
版次1
doihttps://doi.org/10.1007/978-94-009-5468-7
isbn_softcover978-94-010-8914-2
isbn_ebook978-94-009-5468-7Series ISSN 1389-2185
issn_series 1389-2185
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1985
The information of publication is updating

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1389-2185 rt between the chaoticists and astrophysicists at the meeting. We have several introductory papers on chaos in these proceedings, particularly on the analysis o978-94-010-8914-2978-94-009-5468-7Series ISSN 1389-2185
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Book 1985terpretation of observations. But we did not try to conceal that we were also interested in chaos itself, and that made for a pleasant rapport between the chaoticists and astrophysicists at the meeting. We have several introductory papers on chaos in these proceedings, particularly on the analysis o
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V. Gupta,M. D. Lechner,R. Guptasolution . of the evolution equation. There are two implicit assumptions which are usually invoked for analysis of time series data in these terms. The first assumption is that of stationarity. One assumes that observations can be continued forever without significant change of statistical averages.
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1389-2185 n the atom is perhaps the most stunning instance. For us, the deduction of the mean density of a star from its oscillation period is another important example. What then can we deduce about an oscillator that is not periodic? If there are several frequencies or if the behavior is chaotic, may we not
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https://doi.org/10.1007/978-3-642-41556-2ay burst sources..When the impact of the burst luminosity on the accretion rate is introduced, the system is shown to exhibit a complex temporal behaviour. As the basic accretion rate is increased, the system undergoes a sequence of bifurcations, starting from strictly periodic bursts and finally reaching a chaotic behavior.
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