Titlebook: Cosmic Ray Astrophysics; Reinhard Schlickeiser Textbook 2002 Springer-Verlag Berlin Heidelberg 2002 astrophysics.cosmic ray.cosmic rays.el

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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

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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.

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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

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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