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Titlebook: Cosmic Radiation in Contemporary Astrophysics; Maurice M. Shapiro Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1986 Populati

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書目名稱Cosmic Radiation in Contemporary Astrophysics
編輯Maurice M. Shapiro
視頻videohttp://file.papertrans.cn/239/238887/238887.mp4
叢書名稱Nato Science Series C:
圖書封面Titlebook: Cosmic Radiation in Contemporary Astrophysics;  Maurice M. Shapiro Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1986 Populati
描述This volume is the product of Lecturers in the fourth Course of the International School of Cosmic-Ray Astrophysics held at the Ettore Majorana Center in Erice, Sicily in November, 1984. The Course, devoted to "Cosmic Radiation in Contemporary Astrophysics," was concurrently a NATO-sponsored Advanced Study Institute (ASI). Cosmic-ray research is in a state of ferment. Precise measure- ments - some made with instruments aboard sattelites and space probe- have been confronting models and theories with severe constraints. The observations of gamma-ray sources, notably Cyg X-3, at energies up to 16 10 eV, have opened up tantalizing possibilities of direct source iden- tification. This ASI was devoted largely to interdisciplinary phenomena in cosmic-ray astrophysics whose understanding requires input from the other channels in astronomy. It explored the ways in which progress in cosmic-ray science might clarify phenomena observed in related disciplines. In trying to achieve this aim, we assembled a staff of lecturers representing various astrophysical specialties, such as radio- astronomy, optical astronomy, X-ray astronomy, gamma-ray astronomy, and of course, particle astronomy (i.e.,
出版日期Book 1986
關(guān)鍵詞Population; Quasar; astronomy; astrophysics; cosmic ray; instruments; neutron star; quasars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-5488-5
isbn_softcover978-94-010-8922-7
isbn_ebook978-94-009-5488-5Series ISSN 1389-2185
issn_series 1389-2185
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1986
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978-94-010-8922-7D. Reidel Publishing Company, Dordrecht, Holland 1986
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Digital Work: An Organizational Perspectivenergy gain is directly proportional to the product of the strength of the pre-merging magnetic field and the plasma resistivity. Particle acceleration to relativistic energies is possible provided that plasma turbulence or some form of instability leads to a drastic reduction of the classical (Coulo
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A Fair Wage for Workers On-demand via Appand elemental source composition has to be inferred from the observed composition near the earth. The uncertainty in the inferred source composition is largely due to uncertainties in cross sections—especially for nuclides that have large secondary components. These uncertainties will be explored by
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A Fair Wage for Workers On-demand via Apporigin and propagation. The conclusions drawn are as follows. The bulk of cosmic rays detected at earth appear to be of Galactic origin, many probably having come from supernova remnants, at least at the lowest energies. Only above 10.eV does an extragalactic origin appear likely and here the VIRGO
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