標(biāo)題: Titlebook: Cosmic Ray Astrophysics; Reinhard Schlickeiser Textbook 2002 Springer-Verlag Berlin Heidelberg 2002 astrophysics.cosmic ray.cosmic rays.el [打印本頁] 作者: patch-test 時(shí)間: 2025-3-21 20:09
書目名稱Cosmic Ray Astrophysics影響因子(影響力)
書目名稱Cosmic Ray Astrophysics影響因子(影響力)學(xué)科排名
書目名稱Cosmic Ray Astrophysics網(wǎng)絡(luò)公開度
書目名稱Cosmic Ray Astrophysics網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Cosmic Ray Astrophysics被引頻次
書目名稱Cosmic Ray Astrophysics被引頻次學(xué)科排名
書目名稱Cosmic Ray Astrophysics年度引用
書目名稱Cosmic Ray Astrophysics年度引用學(xué)科排名
書目名稱Cosmic Ray Astrophysics讀者反饋
書目名稱Cosmic Ray Astrophysics讀者反饋學(xué)科排名
作者: 取回 時(shí)間: 2025-3-21 21:32
Water Science and Technology Libraryce observable electromagnetic radiation they continuously lose energy and that should affect their propagation and their original energy spectrum. Second, we want to establish the relation between the observable electromagnetic radiation spectra and properties of the radiating particles. Armed with 作者: SOW 時(shí)間: 2025-3-22 03:01
The Crex Crex Collective,Bob Jicklinge convective motion of the medium. As a consequence, the electromagnetic fields in the system are severely influenced by the cosmic ray particles, and the description of cosmic ray transport and acceleration is more complex than solving the equation of motion of charged cosmic ray test particles in 作者: goodwill 時(shí)間: 2025-3-22 07:59
Interactions of Cosmic Ray Electrons,ce observable electromagnetic radiation they continuously lose energy and that should affect their propagation and their original energy spectrum. Second, we want to establish the relation between the observable electromagnetic radiation spectra and properties of the radiating particles. Armed with 作者: exercise 時(shí)間: 2025-3-22 12:16
Acceleration and Transport Processes of Cosmic Rays,e convective motion of the medium. As a consequence, the electromagnetic fields in the system are severely influenced by the cosmic ray particles, and the description of cosmic ray transport and acceleration is more complex than solving the equation of motion of charged cosmic ray test particles in 作者: jaunty 時(shí)間: 2025-3-22 14:43
Textbook 2002the book is primarily of interest to scientists working at the forefront of research, the very careful derivations and explanations make it suitable also as an introduction to the field of cosmic rays for graduate students.作者: jaunty 時(shí)間: 2025-3-22 18:36
Introduction,tude above 5 km, and by noon the group was landing at Pieskow, some 50 km from Berlin. During the six hours of flight Hess had carefully recorded the readings of three electroscopes he used to measure the intensity of radiation and had noted a rise in the radiation level as the balloon rose in altitude.作者: Inoperable 時(shí)間: 2025-3-22 23:25
Statistical Mechanics of Charged Particles, neutral (on the average) system of charged and neutral particles interacting with each other and with an external magnetic field. A gas containing so many free charged particles that their collective Lorentz forces influence the properties of the medium considerably is referred to as a ..作者: 受人支配 時(shí)間: 2025-3-23 02:59
Test Wave Approach 1. Waves in Cold Magnetized Plasmas,e next chapter we are ready to investigate the situation characteristics for cosmic rays in space plasmas, where relativistic cosmic rays co-exist with a background interstellar or intergalactic plasma.作者: 世俗 時(shí)間: 2025-3-23 06:40 作者: 展覽 時(shí)間: 2025-3-23 11:52
Interplanetary Transport of Cosmic Ray Particles,etry properties with respect to the uniform background magnetic field, the calculation of the cosmic ray transport parameters simplifies enormously under the diffusion approximation, as shown in Chap. 13.作者: 口味 時(shí)間: 2025-3-23 15:16 作者: Negligible 時(shí)間: 2025-3-23 21:19 作者: 抗生素 時(shí)間: 2025-3-23 22:44
Immediate Consequences of Galactic Cosmic Ray Observations,l nucleons exhibit power law energy spectra over a wide range of kinetic energies. Cosmic ray electrons exhibit a break in their power law energy spectrum at about 20 GeV with spectral index ? 2.2 below the break energy and ? 3.2 above the break energy.作者: commune 時(shí)間: 2025-3-24 03:24 作者: Spartan 時(shí)間: 2025-3-24 10:19
Sergio Ilarri,Pedro Roig,Raquel Trillo neutral (on the average) system of charged and neutral particles interacting with each other and with an external magnetic field. A gas containing so many free charged particles that their collective Lorentz forces influence the properties of the medium considerably is referred to as a ..作者: Feedback 時(shí)間: 2025-3-24 12:03
Dario Asprone,Sergio Di Martino,Paola Festae next chapter we are ready to investigate the situation characteristics for cosmic rays in space plasmas, where relativistic cosmic rays co-exist with a background interstellar or intergalactic plasma.作者: 保守黨 時(shí)間: 2025-3-24 15:05 作者: Herd-Immunity 時(shí)間: 2025-3-24 20:35
The Crex Crex Collective,Bob Jicklingetry properties with respect to the uniform background magnetic field, the calculation of the cosmic ray transport parameters simplifies enormously under the diffusion approximation, as shown in Chap. 13.作者: 疏忽 時(shí)間: 2025-3-25 01:57 作者: obnoxious 時(shí)間: 2025-3-25 07:19
0941-7834 ludes supplementary material: This book provides an exhaustive account of the origin and dynamics of cosmic rays. Divided into three parts, it first gives an up-to-date summary of the observational data, then -- in the following theory section -- deals with the kinetic description of cosmic ray plas作者: 細(xì)菌等 時(shí)間: 2025-3-25 08:47 作者: prodrome 時(shí)間: 2025-3-25 14:32
ron radiation in the radio wavelength band and for cosmic ray nuclei emission at γ-ray frequencies are most decisive. In the following we describe the results from radio and γ-ray astronomy concerning the origin of cosmic rays.作者: frivolous 時(shí)間: 2025-3-25 17:44 作者: ACME 時(shí)間: 2025-3-25 23:02
W?odzimierz Marszelewski,Bo?ena Pius the cross-sections of electromagnetic interactions of cosmic ray nucleus are much smaller than those of the cosmic ray electrons of the same Lorentz factor, and can be neglected in practically all astrophysical applications as production processes for cosmic photons and as energy loss processes for cosmic ray nuclei.作者: 專心 時(shí)間: 2025-3-26 00:32
Interactions of Cosmic Ray Nuclei, the cross-sections of electromagnetic interactions of cosmic ray nucleus are much smaller than those of the cosmic ray electrons of the same Lorentz factor, and can be neglected in practically all astrophysical applications as production processes for cosmic photons and as energy loss processes for cosmic ray nuclei.作者: 恃強(qiáng)凌弱 時(shí)間: 2025-3-26 07:21
Introduction,a series of seven launches. The flight, which had started at Aussig on the river Elbe, was under the command of Captain W. Hoffory. The meteorological observer was W. Wolf and Hess listed himself as “observer for atmospheric electricity”. Over the next three or four hours the balloon rose to an alti作者: 精確 時(shí)間: 2025-3-26 08:31
Cosmic Rays as Part of the Universe,electrons, positrons and nucleons with kinetic energies greater than 1 keV that bombards the Earth from outside. To understand the origin and dynamics of these particles we have to recall some basic astronomical observations concerning the structure and content of the universe.作者: chuckle 時(shí)間: 2025-3-26 16:33 作者: 鐵砧 時(shí)間: 2025-3-26 17:22 作者: Mast-Cell 時(shí)間: 2025-3-26 22:26 作者: Electrolysis 時(shí)間: 2025-3-27 03:59 作者: Cumbersome 時(shí)間: 2025-3-27 07:01 作者: 指數(shù) 時(shí)間: 2025-3-27 10:40
Statistical Mechanics of Charged Particles, their mutual interactions via electromagnetic fields, generated and maintained by their own streaming, is of particular importance not only for the cosmic rays but also the other components of the interstellar and intergalactic media. In this chapter we will consider the behavior of an electrically作者: Rinne-Test 時(shí)間: 2025-3-27 16:26 作者: Bridle 時(shí)間: 2025-3-27 21:28
Test Wave Approach 2. Waves in Hot Magnetized Isotropic Plasmas,initial transit period, will consist of a spectrum of normal modes at different wavenumbers, see (8.3.42). After discussing the cold plasma limit in the last chapter we now turn our attention to hot plasmas.作者: 巨頭 時(shí)間: 2025-3-28 01:40 作者: orthopedist 時(shí)間: 2025-3-28 03:34 作者: AXIOM 時(shí)間: 2025-3-28 08:18 作者: Immobilize 時(shí)間: 2025-3-28 13:36
Reinhard SchlickeiserThis is the only modern book on the market.All competitive titles date back to 1990 and do not take the latest developments into account.Includes supplementary material: 作者: Obstacle 時(shí)間: 2025-3-28 16:30
Astronomy and Astrophysics Libraryhttp://image.papertrans.cn/c/image/238889.jpg作者: 好色 時(shí)間: 2025-3-28 20:22
https://doi.org/10.1007/978-3-319-79014-5a series of seven launches. The flight, which had started at Aussig on the river Elbe, was under the command of Captain W. Hoffory. The meteorological observer was W. Wolf and Hess listed himself as “observer for atmospheric electricity”. Over the next three or four hours the balloon rose to an alti作者: 束縛 時(shí)間: 2025-3-29 02:53
https://doi.org/10.1007/978-3-319-79014-5electrons, positrons and nucleons with kinetic energies greater than 1 keV that bombards the Earth from outside. To understand the origin and dynamics of these particles we have to recall some basic astronomical observations concerning the structure and content of the universe.作者: tendinitis 時(shí)間: 2025-3-29 03:43
Liliana Zaharia,Gabriela Ioana-Toroimacht solid-state particle detectors, which was achieved after World War II, the original ground-based cosmic ray airshower experiments were supplemented by in situ measurements of the cosmic ray flux in the interplanetary space. Today, detectors on board spacecraft routinely provide spatial and tempor作者: 神秘 時(shí)間: 2025-3-29 09:52 作者: 留戀 時(shí)間: 2025-3-29 15:29 作者: Extort 時(shí)間: 2025-3-29 17:53 作者: conjunctivitis 時(shí)間: 2025-3-29 22:27 作者: neutrophils 時(shí)間: 2025-3-30 02:51 作者: 吸氣 時(shí)間: 2025-3-30 06:50
Dario Asprone,Sergio Di Martino,Paola Festainitial transit period, will consist of a spectrum of normal modes at different wavenumbers, see (8.3.42). In the following we will discuss the resulting plasma waves for different assumed initial configurations of magnetized plasma. After treating plasma waves in cold and hot plasmas in this and th作者: 接觸 時(shí)間: 2025-3-30 11:54 作者: 壁畫 時(shí)間: 2025-3-30 14:56 作者: 身心疲憊 時(shí)間: 2025-3-30 17:48
The Crex Crex Collective,Bob Jickling energetic charged particles, i.e. the cosmic rays. The in-situ study of these transport and acceleration processes in interplanetary space offers a unique opportunity to test our conceptual understanding of cosmic ray dynamics, and thus provides an increased confidence in the applicability of the d作者: Extemporize 時(shí)間: 2025-3-30 22:47
The Crex Crex Collective,Bob Jicklingatistical properties of the electromagnetic fluctuations in this system, expressed through the correlation tensors of the electric and magnetic field fluctuations (12.2.6). If these electromagnetic fluctuations can be identified with normal low-frequency plasma wave modes and/or exhibit certain symm作者: 負(fù)擔(dān) 時(shí)間: 2025-3-31 04:21 作者: 毗鄰 時(shí)間: 2025-3-31 06:33
