標(biāo)題: Titlebook: Nonlinear Phenomena in Stellar Variability; M. Takeuti,J.-R. Buchler Book 1993 Springer Science+Business Media Dordrecht 1993 Accretion.Va [打印本頁(yè)] 作者: Abeyance 時(shí)間: 2025-3-21 18:42
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability影響因子(影響力)
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability被引頻次
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability被引頻次學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability年度引用
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability年度引用學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability讀者反饋
書(shū)目名稱(chēng)Nonlinear Phenomena in Stellar Variability讀者反饋學(xué)科排名
作者: commonsense 時(shí)間: 2025-3-21 22:52
Characterisation of the Dynamics of a Variable StarTentatives to detect chaos in variable stars are presented. Constraints on the accuracy on individual measurements and length of the records, necessary to obtain de-fenitive conclusions, are discussed. Some directions for future improvements are sketched.作者: 詞匯 時(shí)間: 2025-3-22 00:27 作者: 大炮 時(shí)間: 2025-3-22 06:46 作者: 四目在模仿 時(shí)間: 2025-3-22 10:28
Variability of X-Ray Emission from Cen X-3 Observed with GingaSimplified stellar models like as one-zone models can be oscillated in chaotic state (Saitou . 1989). It is natural to consider that the irregular variations of Galactic X-ray sources might be caused from nonlinear oscillation of accretion disks or related flow. We studied the variability of Cen X-3 for applying the nonlinear theory to it.作者: AVOW 時(shí)間: 2025-3-22 13:59 作者: reflection 時(shí)間: 2025-3-22 17:44 作者: expdient 時(shí)間: 2025-3-22 22:04
Nonlinear Expansion Triggered by Magnetic Stress in Accretion Flow onto a Black Holeonlinear effects in the accretion flow accelerate the rate of expansion of the Alfven mode. The accretion flow becomes unstable at the weak strength of magnetic field which is about one-thirtieth of the expected value by the linear theory.作者: 疼死我了 時(shí)間: 2025-3-23 02:24 作者: 聽(tīng)寫(xiě) 時(shí)間: 2025-3-23 06:58 作者: 放牧 時(shí)間: 2025-3-23 12:47 作者: Rotator-Cuff 時(shí)間: 2025-3-23 14:41
Predicting Variable Star Light Curvestion method which exploits the dynamical system theory. A method for filling gaps in data has thereby been constructed. Estimated bounds to the necessary embedding dimension can be obtained and chaotic divergences can be estimated.作者: Enrage 時(shí)間: 2025-3-23 18:39 作者: Servile 時(shí)間: 2025-3-23 23:52
http://image.papertrans.cn/n/image/667643.jpg作者: 新手 時(shí)間: 2025-3-24 05:45
https://doi.org/10.1007/978-94-011-1062-4Accretion; Variation; accretion disk; active galactic nuclei; black hole; black holes; planet; star; stellar作者: FRONT 時(shí)間: 2025-3-24 07:12 作者: 入會(huì) 時(shí)間: 2025-3-24 14:02
M. Takeutirough understanding of the diseases and disorders affecting the pediatric central nervous system is vital for any physician or healthcare provider working in the PICU. In the following pages, an international panel of experts provides an in-depth discussion on the res- citation, stabilization, and o作者: 注視 時(shí)間: 2025-3-24 15:07 作者: HAIL 時(shí)間: 2025-3-24 19:43 作者: expire 時(shí)間: 2025-3-25 03:05 作者: venous-leak 時(shí)間: 2025-3-25 04:33 作者: lactic 時(shí)間: 2025-3-25 10:43
W. Unno,D.-R. Xiongt Roman Empire, later called Byzantium. Thus the territory became Christianized by the Orthodox Church. In the late fourteenth century (1385) Albania came under Ottoman rule. Nevertheless, this domination was never complete and the Albanian history since that time until independence is full of revol作者: 我的巨大 時(shí)間: 2025-3-25 14:51 作者: CARK 時(shí)間: 2025-3-25 18:37
Y. Nakamura,T. Ishizukapart of the West Roman Empire. Thus, Catholicism was introduced in this territory. During the Middle Ages Venice became very influential on the Dalmatian coast, and shaped the course of history of many coastal cities, although most were of ancient Greek or Roman origin. During the Middle Ages a King作者: hidebound 時(shí)間: 2025-3-25 22:50 作者: 玩笑 時(shí)間: 2025-3-26 01:09
R. Kanetake,T. Takeshima,K. Makishima,M. Takeuti the influencing mechanism of acoustic environment on urban .The main focus of this monograph is urban acoustic environment of urban spatial morphology.It provides in-depth evaluation and research on the correlation between urban spatial morphology indicator and urban acoustic environment using urba作者: Melanocytes 時(shí)間: 2025-3-26 07:49
K. Tainaka,S. Fukazawa,H. Nishimori,M. Yokosawa,S. Mineshigeronment. As pointed out above, urban thermal environment has scale characteristics. Therefore, it is particularly important to explore the influence mechanism of urban form indexes on thermal environment on different scales thus to lead thermal environment via urban form control, improve outdoor the作者: 蛙鳴聲 時(shí)間: 2025-3-26 09:16 作者: MAG 時(shí)間: 2025-3-26 15:23
J. R. Percyronment. As pointed out above, urban thermal environment has scale characteristics. Therefore, it is particularly important to explore the influence mechanism of urban form indexes on thermal environment on different scales thus to lead thermal environment via urban form control, improve outdoor the作者: START 時(shí)間: 2025-3-26 16:51 作者: Obverse 時(shí)間: 2025-3-26 22:40
D. Barthés,Y. Tuchman,M. O. Mennessier,J. A. Matteiving environment to a certain extent and led to the increasingly serious urban environmental problems. At the same time, with the continuous improvement of living standards, people’s demands for quality of life have also been correspondingly raised. Urban space environment has the closest relationsh作者: 禁止,切斷 時(shí)間: 2025-3-27 01:39
Z. Kolláthving environment to a certain extent and led to the increasingly serious urban environmental problems. At the same time, with the continuous improvement of living standards, people’s demands for quality of life have also been correspondingly raised. Urban space environment has the closest relationsh作者: Angioplasty 時(shí)間: 2025-3-27 09:14 作者: 縮影 時(shí)間: 2025-3-27 10:40
A Dynamical Systems Approach to Nonlinear Stellar Pulsationsodynamics this approach provides a more fundamental understanding of the systematics of the pulsational behavior. For weakly nonadiabatic pulsations, whether regular or multi-periodic, dimensional reduction techniques lead to amplitude equations and to a description in terms of modal interactions an作者: BANAL 時(shí)間: 2025-3-27 14:33
Patterns of Aperiodic Pulsationation of a map for the patterns of pulsation phases is described. This map gives the time between two successive maxima of pulsation in terms of the time between the previous pair, under suitable conditions. The phase differences can be regular, chaotic or hyperchaotic.作者: 硬化 時(shí)間: 2025-3-27 20:38
Non-Linear Oscillations and Beats in the Beta Canis Majoris Starsris stars, no one of these does it satisfactorily. Possibly it is due to an inadequate elaboration of the non-Iinearly oscillation theory. Analysis and critical evaluation of the existing hypotheses are given by Mel’nikov and Popov (1970). Our explanation consists in existence of close frequencies c作者: NEEDY 時(shí)間: 2025-3-27 23:49 作者: SPALL 時(shí)間: 2025-3-28 02:33 作者: 執(zhí) 時(shí)間: 2025-3-28 09:38 作者: acrobat 時(shí)間: 2025-3-28 14:21 作者: Shuttle 時(shí)間: 2025-3-28 16:26 作者: Ballad 時(shí)間: 2025-3-28 19:39 作者: FUSC 時(shí)間: 2025-3-28 23:41 作者: 聽(tīng)覺(jué) 時(shí)間: 2025-3-29 03:09
Predicting Variable Star Light Curvestion method which exploits the dynamical system theory. A method for filling gaps in data has thereby been constructed. Estimated bounds to the necessary embedding dimension can be obtained and chaotic divergences can be estimated.作者: 用手捏 時(shí)間: 2025-3-29 09:31 作者: ordain 時(shí)間: 2025-3-29 12:45 作者: 我們的面粉 時(shí)間: 2025-3-29 16:50 作者: Inflated 時(shí)間: 2025-3-29 21:31 作者: 斷言 時(shí)間: 2025-3-30 03:46
the estimate of stability, the appearance and disappearance of possible modes can be studied in detail. While nonlinearity in stellar pulsations is not a very complicated concept, it generally requires extensive and sometimes so- phisticated numerical studies. Therefore, the development of appropri作者: 武器 時(shí)間: 2025-3-30 05:58 作者: Flatus 時(shí)間: 2025-3-30 10:05
J. R. Buchlerndous advances in the understanding of critical illness have been realized in the last decade. My family has directly bene? ted from some of the technological and scienti? c advances made in the care of critically ill children. My son Ryan was born during my third year of medical school. By some pec作者: Compass 時(shí)間: 2025-3-30 14:43 作者: nepotism 時(shí)間: 2025-3-30 18:47 作者: 精密 時(shí)間: 2025-3-31 00:26
R. Kanetake,T. Takeshima,K. Makishima,M. Takeutiroclimate simulation by using Cadna/A acoustic simulation software. It concludes the influencing mechanism of acoustic environment on urban morphology. It makes a valuable contribution for the research on urban environment and urban morphology...?.978-981-13-9704-2978-981-13-9702-8作者: 羊齒 時(shí)間: 2025-3-31 04:43 作者: Derogate 時(shí)間: 2025-3-31 08:05 作者: goodwill 時(shí)間: 2025-3-31 11:43 作者: 情節(jié)劇 時(shí)間: 2025-3-31 14:48
