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Titlebook: Neural Network Dynamics; Proceedings of the W J. G. Taylor (Director),E. R. Caianiello,J. W. Cla Conference proceedings 1992 Springer-Verla

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发表于 2025-3-21 19:52:41 | 显示全部楼层 |阅读模式
书目名称Neural Network Dynamics
副标题Proceedings of the W
编辑J. G. Taylor (Director),E. R. Caianiello,J. W. Cla
视频video
丛书名称Perspectives in Neural Computing
图书封面Titlebook: Neural Network Dynamics; Proceedings of the W J. G. Taylor (Director),E. R. Caianiello,J. W. Cla Conference proceedings 1992 Springer-Verla
描述.Neural Network Dynamics. is the latest volume in the .Perspectives in Neural Computing. series. It contains papers presented at the 1991 Workshop on Complex Dynamics in Neural Networks, held at IIASS in Vietri, Italy. The workshop encompassed a wide range of topics in which neural networks play a fundamental role, and aimed to bridge the gap between neural computation and computational neuroscience. The papers - which have been updated where necessary to include new results - are divided into four sections, covering the foundations of neural network dynamics, oscillatory neural networks, as well as scientific and biological applications of neural networks. Among the topics discussed are: A general analysis of neural network activity; Descriptions of various network architectures and nodes; Correlated neuronal firing; A theoretical framework for analyzing the behaviour of real and simulated neuronal networks; The structural properties of proteins; Nuclear phenomenology; Resonance searches in high energy physics; The investigation of information storage; Visual cortical architecture; Visual processing. .Neural Network Dynamics. is the first volume to cover neural networks and comput
出版日期Conference proceedings 1992
关键词artificial intelligence; associative memory; behavior; cognition; computational neuroscience; cortex; memo
版次1
doihttps://doi.org/10.1007/978-1-4471-2001-8
isbn_softcover978-3-540-19771-3
isbn_ebook978-1-4471-2001-8Series ISSN 1431-6854
issn_series 1431-6854
copyrightSpringer-Verlag London Limited 1992
The information of publication is updating

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Günther Palm,Friedrich T. Sommeranet formation therefore can.be studied in a static nebula.in a nebula evolving from an arbitrary initial condition. We propose a simple approach to both account for sedimentation from the molecular cloud onto the disk, disk evolution and migration of solids..Giant planets have key roles in the hist
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Denise Gorseg with the interior nebula, for long periods of time. It seems more likely that hydrodynamic outflow is actually established below this zone, in the body of the disk. In this case fractionations are governed by Rayleigh distillation of the entire remaining nebula, and are negligible at the time when
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Karl E. Kürten surfaces are continuously bombarded by energetic ions from solar wind and flares, planetary magnetospheres and galactic cosmic rays. Many applications of the above type of experiments have been discussed in recent years and are here reviewed. These include modifications undergone by comets and sate
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Paul C. Bressloffelengths characteristic of the molecules of gas of which it is composed The molecules are found to be ionised, consisting mainly of CO., H.O., OH.. The dominant ion CO. gives the tail its characteristic blue appearance in photographs. Since the particles are charged the second tail is known as the p
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