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Titlebook: Electromagnetic Radiation in Space; Proceedings of the T J. G. Emming Conference proceedings 1967 D. Reidel Publishing Company, Dordrecht,

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书目名称Electromagnetic Radiation in Space
副标题Proceedings of the T
编辑J. G. Emming
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Electromagnetic Radiation in Space; Proceedings of the T J. G. Emming Conference proceedings 1967 D. Reidel Publishing Company, Dordrecht,
描述The subject of this volume in the Astrophysics and Space Science Library is Electro­ magnetic Radiation in Space. It is essentially based on the lectures given at the third ESRO Summer School which was held from 19 July to 13 August, 1965, in Alpbach, Austria. Fifty-eight selected students attended the courses representing the following countries: Austria (2), Belgium (1), Denmark (1), France (12), Germany (10), Italy (7), Netherlands (2), Spain (4), Sweden (6), Switzerland (3), United Kingdom (9), United States (1). Thirteen lectures courses and nine seminars were given by sixteen different scientists in total. In this book the courses and seminars have been classified in three parts according to the kind of radiation which they mainly deal with: Ultraviolet Radiation, X­ Radiation and Cosmic Radiation. These parts can be broken down further in theo­ retical and observational aspects, whereas in the first and second part solar as well as stellar ultraviolet- and X-radiation can be distinguished. * Due to various reasons the publication of this volume had to be delayed; it was therefore judged appropriate to bring the text up to date. The various lecturers have been asked to revise
出版日期Conference proceedings 1967
关键词astronomy; astrophysics; cosmic ray; solar; space physics
版次1
doihttps://doi.org/10.1007/978-94-010-3526-2
isbn_softcover978-94-010-3528-6
isbn_ebook978-94-010-3526-2Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1967
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Ultraviolet Astronomy: Observational Aspectsomy. No hard and fast demarcation can be drawn and a considerable region of overlap exists, including, for example, the moon and planets. There is a basic difference between the two subjects in the experimental sense since most geophysical experiments use the spacecraft as a probe to make measuremen
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Observations of Solar Ultraviolet Radiationcts himself to a brief discussion of the main scientific objectives of present-day solar UV observations. The most important instrumental problems are reviewed. The opinion is stated that several comparatively simple satellites seem to be better suited for investigating the solar UV spectrum than a
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Theoretical Aspects of Solar X-Radiations are of nuclear origin. Mostly gamma rays are harder than X-rays. This distinction has not rigorously been followed in the astronomical literature, and in actual fact, it has sometimes only been the . of the solar quanta that was used to classify them. However, one had better avoid confusion and ke
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Rayons Cosmiques et Rayonnement Synchrotronion en rayons cosmiques et en champs magnétiques est forte, et qui sont probablement des sources de rayons cosmiques. Après avoir revu rapidement les propriétés du rayonnement synchrotron, l’auteur passe en revue les radiosources discrètes, lesquelles émettent toutes par rayonnement synchrotron et s
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