Titlebook: Neural Nets WIRN VIETRI-98; Proceedings of the 1 Maria Marinaro,Roberto Tagliaferri Conference proceedings 1999 Springer-Verlag London Limi

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Allodynia

sample. In particular, the SDD data allow the differential study of the leading and following parts with a temporal resolution of 1.5 hours. In this study, we analyse the equilibrium distance of sunspot groups as well as the evolution of this distance over the lifetime of the groups and the shifts i

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Gianluca Setti,Patrick Thiran,Claudio Serpicok presents the results and findings of the HESPERIA (.H.igh .E.nergy .S.olar .P.article .E.vents fo.r.ecast.i.ng and .A.nalysis) project of the EU HORIZON 2020 programme. It discusses the forecasting operational tools developed within the project, and presents progress to SEP research contributed by

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perspective.Presents most recent state-of-the-art scientifiSolar energetic particles (SEPs) emitted from the Sun are a major space weather hazard motivating the development of predictive capabilities. This book presents the results and findings of the HESPERIA (.H.igh .E.nergy .S.olar .P.article .E

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Limousine

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Francesco Frisone,Pietro G. Morassomajor sources of uncertainties: The atomic and molecular data and the solar irradiance. The cross sections and branching ratios used in this analysis come from many different sources; many of them without any error indications. For this reason, we must confine ourselves to a qualitative indication o

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F. Frisone,P. G. Morasso,G. Iannò,M. Marongiu,P. Vitali,G. Rodrigueze stars. The solar atmosphere is a rich physics laboratory, in which the whole spectrum of radiative, dynamical, and magnetic processes that tranfer energy into space can be observed. As the fundamental processes take place on very small spatial scales, we need high· resolution observations to explo

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Davide Mattera,Francesco Palmierie stars. The solar atmosphere is a rich physics laboratory, in which the whole spectrum of radiative, dynamical, and magnetic processes that tranfer energy into space can be observed. As the fundamental processes take place on very small spatial scales, we need high· resolution observations to explo

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