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Titlebook: Observational Manifestation of Chaos in Astrophysical Objects; Invited talks for a Alexei M. Fridman,Mikhail Ya. Marov,Richard H. Mil Book

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發(fā)表于 2025-3-21 19:18:23 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Observational Manifestation of Chaos in Astrophysical Objects
副標題Invited talks for a
編輯Alexei M. Fridman,Mikhail Ya. Marov,Richard H. Mil
視頻videohttp://file.papertrans.cn/701/700364/700364.mp4
圖書封面Titlebook: Observational Manifestation of Chaos in Astrophysical Objects; Invited talks for a  Alexei M. Fridman,Mikhail Ya. Marov,Richard H. Mil Book
描述On August 2000 in the Lomonosov Moscow State University the first scientific conference dedicated to chaos in the real astronomical systems was held. The most prominent astrophysisists - specialist in the field of stochastic dynamics - attended the conference. A broad scope of the problems related to the observed manifes- tations of chaotic motions in galactic and stellar objects, with the involvement of basic theory and numerical modeling, were addressed. The idea (not so obvious, as we believe, to many astrophysicists) was to show that, while great progress in the field of stochastic mechanics was accomplished, the science of chaos in actually observed systems is only just being born. Basically, the situation described prompted the organizers to hold the meeting in order to discuss chaotic processes in real systems. It seemed worthwhile to begin these introductory remarks with a brief descrip- tion of some events that preceeded the conference. Since actually existing systems are the subject of the natural sciences, and in the latter experiments play the key role, we shall begin our account with the experimental results.
出版日期Book 2002
關(guān)鍵詞Accretion; Orbit; Planet; astrophysics; relativistic jet
版次1
doihttps://doi.org/10.1007/978-94-010-0247-9
isbn_softcover978-94-010-3945-1
isbn_ebook978-94-010-0247-9
copyrightSpringer Science+Business Media Dordrecht 2002
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 22:11:45 | 只看該作者
板凳
發(fā)表于 2025-3-22 02:58:51 | 只看該作者
h a brief descrip- tion of some events that preceeded the conference. Since actually existing systems are the subject of the natural sciences, and in the latter experiments play the key role, we shall begin our account with the experimental results.978-94-010-3945-1978-94-010-0247-9
地板
發(fā)表于 2025-3-22 08:03:15 | 只看該作者
Observational Manifestation of Chaos in Astrophysical ObjectsInvited talks for a
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發(fā)表于 2025-3-22 11:42:37 | 只看該作者
Alexei M. Fridman,Mikhail Ya. Marov,Richard H. Mil
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發(fā)表于 2025-3-22 14:48:28 | 只看該作者
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發(fā)表于 2025-3-22 17:40:19 | 只看該作者
Orbits and Integrals in Self-Consistent Systems,sents a stationary elliptical galaxy of type E5, which is approximately axisymmetric around its longest axis. The orbits are of three main types, box orbits (including box-like orbits), tube orbits and chaotic orbits. The box or box-like and tube orbits are represented by closed invariant curves on
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發(fā)表于 2025-3-23 00:38:40 | 只看該作者
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發(fā)表于 2025-3-23 03:19:57 | 只看該作者
Observing Chaos in External Spiral Galaxies,sidered namely: steep potential gradients, resonances and growing spiral perturbations. Several regions where chaos could be expected are identified such as the very central region, the end of the bar, the start of the main spiral pattern and the termination of strong spiral arms..The main observati
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發(fā)表于 2025-3-23 05:52:51 | 只看該作者
Spectral Analysis of Orbits Via Discrete Fourier Transforms,tegrations of those orbits. The algorithms rely entirely on discrete Fourier transforms. We calibrate the algorithms by applying them to some orbits which were studied earlier using the NAFF method. The new algorithms reproduce the test orbits accurately, satisfy constraints which are consequences o
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