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Titlebook: Neural Nets and Surroundings; 22nd Italian Worksho Bruno Apolloni,Simone Bassis,Francesco Carlo Morab Book 2013 Springer-Verlag Berlin Heid

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Genetic Algorithm Modeling with GPU Parallel Computing Technology inherently parallel, the GPGPU computing paradigm has provided an exploit of the internal training features of the model, permitting a strong optimization in terms of processing performances and scalability.
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Balancing Recall and Precision in Stock Market Predictors Using Support Vector Machinesor machines, which employs recall-precision curves in order to allow a buying action for the trader only when the confidence of the prediction is high. We present an extensive experimental evaluation which compares our trader with several classic competitors.
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A Collaborative Filter Approach to Adaptive Noise Cancellationoth filters allows to reach good performances in terms of convergence and speed. In addition a variable step size is used in order to obtain better performance. Several experimental results, in different reverberant conditions, demonstrate the effectiveness of the proposed approach.
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Book 2013ty (CIS). The book – as well as the workshop-  is organized in three main components, two special sessions and a group of regular sessions featuring different aspects and point of views of artificial neural networks and natural intelligence, also including applications of present compelling interest..
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of solar phenomena. Explanations of what to expect visually from white light, Hydrogen-alpha and Calcium K filters are provided for those new to solar observing, along with essential tips on equipment, observing techniques and the practicalities of drawing at the eyepiece. Time-honored, traditional
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Francesco A. N. Palmieri,Alberto Cavalloe and convective energy transport, the paper concentrates on the Sun and other stars with convective envelopes. In a discussion of the solar magnetic structure, the strong-field / weak-field dichotomy is emphasized, and the importance of the strong fields in the structure of outer stellar atmosphere
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Dario Malchiodiosphere which we call "the solar surface". It is from solar surface observations that we must infer the internal structure and the internal magnetohydrodynamic processes that lead to the multitude of fascinat­ ing phenomena of solar magnetic activity, and from solar surface observations we must also
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