CRUDE 发表于 2025-3-23 09:59:27

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Anonymous 发表于 2025-3-23 16:18:09

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Cytokines 发表于 2025-3-23 18:38:54

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) . 3.- by properties of solar FEP interaction with solar wind matter accompanied with GR generation through decay of neutral pions .

留恋 发表于 2025-3-23 23:05:03

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烦忧 发表于 2025-3-24 03:32:37

Astrophysical Sources of High Energy Particles and Radiation978-94-010-0560-9Series ISSN 1568-2609

Permanent 发表于 2025-3-24 09:14:38

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突变 发表于 2025-3-24 12:01:13

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AV-node 发表于 2025-3-24 16:40:26

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FLIP 发表于 2025-3-24 21:32:49

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.

忍受 发表于 2025-3-24 23:25:26

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 ). Although still incomplete, the theory is able to explain the main characteristi
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查看完整版本: Titlebook: Astrophysical Sources of High Energy Particles and Radiation; Maurice M. Shapiro,Todor Stanev,John P. Wefel Book 2001 Springer Science+Bus