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Author: S.R. Kane
Publisher: Springer Science & Business Media
ISBN: 9401018022
Category : Science
Languages : en
Pages : 424
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Book Description
Proceedings of IAU Symposium No. 68 held in Buenos Aires, Argentina, 11-14 June 1974, organized by the IAU in co-operation with COSPAR
Author: S.R. Kane
Publisher: Springer Science & Business Media
ISBN: 9401018022
Category : Science
Languages : en
Pages : 424
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Book Description
Proceedings of IAU Symposium No. 68 held in Buenos Aires, Argentina, 11-14 June 1974, organized by the IAU in co-operation with COSPAR
Author: A. Bruzek
Publisher: Taylor & Francis
ISBN: 9789027708250
Category : Science
Languages : en
Pages : 238
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Book Description
At the XV. General Assembly of the International Astronomical Union in Sydney 1973, Commission 10 for Solar Activity requested the incoming Organising Committee to establish a small group to recommend a standard nomenclature for solar features and to prepare an illustrated text which would clear the jungle of terms for the benefit of solar physicists as well as of theoreticians and research workers in related fields. The challenge was taken up by the president of Commission 10, Prof. K. O. Kiepenheuer, and his persuasive advocacy has led eventually to the present book. In the course of the work, the declared aim but not the basic purpose was revised. Rather than prepare a list of standard terms, we have preferred to collect together all the terms that appear in current English-language literature. Synonyms and partially overlapping terms are all recorded for the most part without prejudice. Each has been defined as exactly as possible with the hope that in the future they may be used and understood without ambiguity. It would be a step on the road to standardisation if these terms were not re-used for new phenomena. New observations and new theories will lead to reappraisals and redefinitions so the Glossary is intended more as a guide to the present situation than as a rule-book.
Author: M. Dryer
Publisher: Springer Science & Business Media
ISBN: 9400991002
Category : Science
Languages : en
Pages : 543
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Book Description
Informal discussions in 1977 among a number of scientists asso ciated with solar and interplanetary physics revealed a need for a dialogue between the two often-divergent groups. It was clear that the latter group was dependent essentially on the sun for its raison d'etre. On the other hand it was also clear that the former group could benefit in its search for insight vis-a-vis solar activity by looking beyond the shell of the inner corona. Needless to add that the combined solar/interplanetary topic is relevant to astrophysics when one considers stellar winds and binary star flows. It was felt, there fore, that a symposium was essential to bring together, for the first time, leading solar and interplanetary physicists from the interna tional community to discuss and record herein their own research. The fundamental physical processes underlying our own capricious star's activity can be understood only by the coupling of solar and interplan etary topics in an intimate observational and theoretical structure. This book, intended for active research scientists and advanced grad uate students, is an important step in this direction. The background of solar and interplanetary dynamics is provided in Part I (The Life History of Coronal Structures and Fields) and Part II (Coronal and Interplanetary Responses to Long Time Scale Phenomena).
Author:
Publisher: American Geophysical Union
ISBN:
Category :
Languages : en
Pages : 523
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Book Description
Author: International Astronomical Union. Symposium
Publisher:
ISBN:
Category :
Languages : en
Pages : 0
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Book Description
Author: Herbert J. Wiehl
Publisher:
ISBN:
Category : Solar flares
Languages : en
Pages : 120
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Book Description
Author: E.L. Chupp
Publisher: Springer Science & Business Media
ISBN: 9401014965
Category : Science
Languages : en
Pages : 332
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Book Description
Observation of discrete energy electromagnetic emissions from celestial objects in the radio, IR, optical, lN, and X-ray spectral regions has dramatically advanced our know ledge in the field of astrophysics. It is expected that identification of nuclear 'Y-ray line emissions from any cosmic source would also prove to be a powerful new tool for probing the Universe. Since the publication of Morrison's work in 1958, many experiments were carried out searching for evidence of 'Y-ray lines from cosmic sources, however with little success. Only a few positive experimental results have been reported, in spite of an expenditure of considerable effort by many people: in particular, the possible Galactic Center emission line (473 to 530keV) and 'Y-ray lines at several energies (e. g. , 0. 5 MeV and 2. 2 MeV) associated with large solar flares. Both of these observations are unconfirmed by indepen dent observations (ca. 1975). The high energy 'Y-rays (>30MeV) from the Galactic Center are at least partly due to the decay of 1[0 mesons, which are of unique energy (67. 5 MeV) in the 1[0 rest frame only. The reasons for the limited amount of data avail able in this field, even though early theoretical predictions were very optimistic regarding fluxes of nuclear lines, are that experimental efforts are plagued with high backgrounds and low fluxes, and that development of instruments with telescopic properties in the energy range of interest is difficult.
Author: Carl E. Fichtel
Publisher:
ISBN:
Category : Gamma ray astronomy
Languages : en
Pages : 388
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Author:
Publisher:
ISBN:
Category : Naval research
Languages : en
Pages : 1016
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Author: Naval Research Laboratory (U.S.)
Publisher:
ISBN:
Category : Electronics
Languages : en
Pages : 196
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Book Description
