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Titlebook: Astrophysical Sources of High Energy Particles and Radiation; Maurice M. Shapiro,Todor Stanev,John P. Wefel Book 2001 Springer Science+Bus

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樓主: SCOWL
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發(fā)表于 2025-3-23 09:59:27 | 只看該作者
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Variable Gamma Ray Sources, 1: Interactions of Flare Energetic Particles with Solar and Stellar Winds of solar FEP (especially in periods of very great events) [12–14, 15]. 3.- by properties of solar FEP interaction with solar wind matter accompanied with GR generation through decay of neutral pions [16–18].
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發(fā)表于 2025-3-23 23:05:03 | 只看該作者
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Astrophysical Sources of High Energy Particles and Radiation978-94-010-0560-9Series ISSN 1568-2609
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Correlation and ClusteringIn this lecture we clarify the basic difference between the correlation properties for systems characterized by small or large fluctuations. The concepts of correlation length, homogeneity scale, scale invariance and criticality are discussed as well. We relate these concepts to the interpretation of galaxy clsutering.
20#
發(fā)表于 2025-3-24 23:25:26 | 只看該作者
https://doi.org/10.1007/978-1-4302-0103-8 rays (CRs) originates in supernova remnants (SNRs). Theoretically progress in the solution of this problem has been due to the development of the theory of diffusive shock acceleration (see, for example, reviews [1–3]). Although still incomplete, the theory is able to explain the main characteristi
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