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Titlebook: Origin of Cosmic Rays; Giancarlo Setti,Gianfranco Spada,Arnold W. Wolfend Book 1981 International Astronomical Union 1981 active galactic

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發(fā)表于 2025-3-21 17:52:22 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Origin of Cosmic Rays
編輯Giancarlo Setti,Gianfranco Spada,Arnold W. Wolfend
視頻videohttp://file.papertrans.cn/705/704603/704603.mp4
叢書名稱International Astronomical Union Symposia
圖書封面Titlebook: Origin of Cosmic Rays;  Giancarlo Setti,Gianfranco Spada,Arnold W. Wolfend Book 1981 International Astronomical Union 1981 active galactic
描述The cosmic radiation was discovered by Hess in 1912 but its origin is still the subject of much controversy and considerable study. For several decades most workers in the cosmic ray field were interested in the Nuclear Physical aspect of the particle beam and many important dis- coveries were made, notably the identification of the positron, the muon, the pion and the strange particles. More recently however, em- phasis has changed to the Astrophysical aspect both with re8ard to the origin of the radiation and to its relation with the other radiation fields. Mindful of the increasing importance of the Astrophysical facets of the subject the Cosmic Ray Commission of IUPAP approached the High Energy Astrophysics Commission of the IAU with the suggestion of a joint Symposium on Cosmic Ray Origin. The plan was to bring together workers in all the various astronomical fields - from Radio, through Optical to Gamma Rays - with Cosmic Ray physicists and to fully explore the various interrelations. The approach was received with enthusiasm and this book contains the proceedings of the ensuing Symposium, (styled IUPAP/ IAU Symposium No. 94) which was held in Bologna from 11th - 14th June 19
出版日期Book 1981
關(guān)鍵詞active galactic nuclei; astrophysics; cosmic ray; heliosphere; interstellar matter; quasar; star; star form
版次1
doihttps://doi.org/10.1007/978-94-009-8475-2
isbn_softcover978-90-277-1272-1
isbn_ebook978-94-009-8475-2Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightInternational Astronomical Union 1981
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 22:46:55 | 只看該作者
978-90-277-1272-1International Astronomical Union 1981
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International Astronomical Union Symposiahttp://image.papertrans.cn/o/image/704603.jpg
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https://doi.org/10.1007/978-94-009-8475-2active galactic nuclei; astrophysics; cosmic ray; heliosphere; interstellar matter; quasar; star; star form
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發(fā)表于 2025-3-22 14:40:40 | 只看該作者
The Origin of Cosmic Rays (Introductory Remarks),The field of study, which by tradition is still called ‘the problem of cosmic ray origin’, is now at a watershed, at a turning point. For this reason the time chosen for the present Symposium is especially suited.
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CR-39 Plastic Track Detector Experiment for Measurement of Charge Composition of Primary Cosmic Rays of stack assembly was adopted for these modules: one consisting of ‘pure’ CR-39 plastic track detector: the next one, a composite assembly of CR-39 with three layers of 600 micron thick nuclear emulsions: and the last one with CR-39 and Lexan Polycarbonate. The payload was flown successfully in Ju
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發(fā)表于 2025-3-23 07:32:05 | 只看該作者
Interstellar and Intracluster Tunnels and Acceleration of High-Energy Cosmic Rays,ed by single sources into interstellar space undergo momentum diffusion by stochastic interaction with long wavelength MHD perturbations; small wavelength modes provide pitchangle scatterings. These MHD perturbations, A Ifvèn and fast magnetosonic waves, are generated by the dynamic interaction of s
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