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Titlebook: Genesis and Propagation of Cosmic Rays; Maurice M. Shapiro (Director of the School, Co-Dir Book 1988 D. Reidel Publishing Company, Dordrec

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發(fā)表于 2025-3-21 18:29:25 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Genesis and Propagation of Cosmic Rays
編輯Maurice M. Shapiro (Director of the School, Co-Dir
視頻videohttp://file.papertrans.cn/383/382426/382426.mp4
叢書名稱Nato Science Series C:
圖書封面Titlebook: Genesis and Propagation of Cosmic Rays;  Maurice M. Shapiro (Director of the School, Co-Dir Book 1988 D. Reidel Publishing Company, Dordrec
出版日期Book 1988
關(guān)鍵詞active galactic nuclei; astronomy; astrophysics; cosmic ray; earth; heliosphere; observatory; radio astrono
版次1
doihttps://doi.org/10.1007/978-94-009-4025-3
isbn_softcover978-94-010-8286-0
isbn_ebook978-94-009-4025-3Series ISSN 1389-2185
issn_series 1389-2185
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1988
The information of publication is updating

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發(fā)表于 2025-3-21 21:53:30 | 只看該作者
Stars and Cosmic Rays,e review our current knowledge on “solarlike activity” and its relation with stellar parameters at various locations of the Hertzsprung-Russell diagram. This “solar-stellar connection” emphasizes the role of solar studies in helping to understand the pre-acceleration states of the history of galactic cosmic rays.
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發(fā)表于 2025-3-22 03:35:30 | 只看該作者
Conditions for Acceleration of Super-High Energy Cosmic Rays in Active Galactic Nuclei,a low impedance element (ambient conducting medium). Beam particles can be accelerated to 10. provided that the beam channel medium behaves like an inductive circuit with high impedance. But even if these conditions are satisfied, a major difficulty the model faces is the large energy loss caused by photomeson reactions.
地板
發(fā)表于 2025-3-22 06:02:08 | 只看該作者
Cosmic Ray Bombardment of Solids in Space,ant role played in giant molecular clouds by cosmic rays for the production of molecular hydrogen, the cornerstone of interstellar chemistry. A method to obtain suitable information on the almost unknown spectrum of low energy cosmic rays outside the heliosphere is also presented.
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發(fā)表于 2025-3-22 12:16:41 | 只看該作者
Current Issues in Macroeconomics sky area. Events with energy above 5×10. eV are largely of extragalactic origin. Several particles arrive preferentialy from the general direction of the local supercluster. There is also an excess of particles coming from the Galactic South Pole direction, which is not understood.
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發(fā)表于 2025-3-22 15:36:20 | 只看該作者
Current Issues in Maritime Economicse review our current knowledge on “solarlike activity” and its relation with stellar parameters at various locations of the Hertzsprung-Russell diagram. This “solar-stellar connection” emphasizes the role of solar studies in helping to understand the pre-acceleration states of the history of galactic cosmic rays.
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發(fā)表于 2025-3-22 22:21:40 | 只看該作者
Elling Prediction in Ocular Pursuit,ant role played in giant molecular clouds by cosmic rays for the production of molecular hydrogen, the cornerstone of interstellar chemistry. A method to obtain suitable information on the almost unknown spectrum of low energy cosmic rays outside the heliosphere is also presented.
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發(fā)表于 2025-3-23 04:12:06 | 只看該作者
Enrico G. Beltrametti,Bas C. Fraassenhese results are then compared with the measured properties of the e. component of cosmic rays in the solar neighborhood. It is found that even though this component of the cosmic rays is a rather minor one in terms of either number or energetics, it is the component which appears best explained by known phenomena at the present time.
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發(fā)表于 2025-3-23 09:09:10 | 只看該作者
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