標(biāo)題: Titlebook: Nonlinear Cosmic Ray Diffusion Theories; Andreas Shalchi Book 2009 Springer-Verlag Berlin Heidelberg 2009 Cosmic Rays.Diffusion Theory.Dif [打印本頁(yè)] 作者: DEBUT 時(shí)間: 2025-3-21 17:54
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories影響因子(影響力)
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories被引頻次
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories被引頻次學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories年度引用
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories年度引用學(xué)科排名
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories讀者反饋
書(shū)目名稱(chēng)Nonlinear Cosmic Ray Diffusion Theories讀者反饋學(xué)科排名
作者: 鐵砧 時(shí)間: 2025-3-21 21:48
0067-0057 ble for the high cosmic ray energies that have been observed. The layout of this book is as follows. In Chap. 1, the general physical scenario is presented. We discuss fundamental processes such as cosmic ray propagation and accelerati978-3-642-10139-7978-3-642-00309-7Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 場(chǎng)所 時(shí)間: 2025-3-22 01:04
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/n/image/667380.jpg作者: 狂熱文化 時(shí)間: 2025-3-22 07:38
https://doi.org/10.1007/978-3-642-00309-7Cosmic Rays; Diffusion Theory; Diffusive Shock Acceleration; Interstellar Medium; Nonlinear Transport Th作者: Aviary 時(shí)間: 2025-3-22 12:15 作者: cutlery 時(shí)間: 2025-3-22 15:52
Nonlinear Cosmic Ray Diffusion Theories978-3-642-00309-7Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 小說(shuō) 時(shí)間: 2025-3-22 20:00
Andreas ShalchiA science monograph presenting the forefront of cosmic ray diffusion theory作者: 6Applepolish 時(shí)間: 2025-3-22 23:34
0067-0057 lar medium, they interact with a large-scale magnetic ?eld such as the magnetic ?eld of the Sun or the Galactic magnetic ?eld. As these background ?elds are usually nearly constant in time and space, they can be approximated by a homogeneous ?eld. If there are no additional ?elds, the particle traje作者: altruism 時(shí)間: 2025-3-23 04:21
Book 2009of the Sun or the Galactic magnetic ?eld. As these background ?elds are usually nearly constant in time and space, they can be approximated by a homogeneous ?eld. If there are no additional ?elds, the particle trajectory is a perfect helix along which the par- cle moves at a constant speed. In reali作者: 改變 時(shí)間: 2025-3-23 06:26
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