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Author : S.R. Kane
Publisher : Springer Science & Business Media
Page : 424 pages
File Size : 41,7 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789401018029
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 : International Astronomical Union. Symposium
Publisher : Unknown
Page : 0 pages
File Size : 43,6 Mb
Release : 1975
Category : Electronic
ISBN : OCLC:896179410
Author : Sharad R. Kane
Publisher : Unknown
Page : 0 pages
File Size : 43,5 Mb
Release : 1975
Category : Solar radiation
ISBN : OCLC:654660646
Author : A. Bruzek,C.J. Durrant
Publisher : Taylor & Francis
Page : 238 pages
File Size : 41,9 Mb
Release : 1977-12-31
Category : Science
ISBN : 9027708258
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,Einar Tandberg-Hanssen
Publisher : Springer Science & Business Media
Page : 543 pages
File Size : 44,8 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400991002
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 : Anonim
Publisher : American Geophysical Union
Page : 523 pages
File Size : 47,8 Mb
Release : 2024-06-29
Category : Electronic
ISBN : 8210379456XXX
Author : Naval Research Laboratory (U.S.)
Publisher : Unknown
Page : 196 pages
File Size : 46,5 Mb
Release : 1976
Category : Electronics
ISBN : IND:30000097131290
Author : Anonim
Publisher : Unknown
Page : 196 pages
File Size : 48,9 Mb
Release : 1975
Category : Naval research
ISBN : WISC:89050408418
Author : Naval Research Laboratory (U.S.)
Publisher : Unknown
Page : 208 pages
File Size : 46,9 Mb
Release : 1975
Category : Naval research
ISBN : IND:30000090196175
Author : Naval Research Laboratory (U.S.)
Publisher : Unknown
Page : 76 pages
File Size : 50,8 Mb
Release : 1975-08
Category : Naval research
ISBN : MINN:31951D03428564D
Author : E. N. Parker
Publisher : Oxford University Press
Page : 860 pages
File Size : 54,7 Mb
Release : 2019-10-10
Category : Science
ISBN : 9780192565570
This well known and widely used landmark text explores the universal spontaneous generation of magnetic fields in astronomical bodies and the agitation of the bodies by those fields. The general properties of magnetic fields, their appearance throughout the astronomical universe, and the havoc they wreak are described in simple physical terms so as to define the broad scientific problem presented by magnetic fields. Then, with the physical problems clearly in mind, the theoretical effects are demonstrated with formal mathematical illustrations from the basic electromagnetic equations. Oxford Classic Texts in the Physical Sciences From James Clerk Maxwell's towering achievement Treatise on electricity and magnetism, to today's ground-breaking research, Oxford University Press has often been regarded as the publisher of first choice for generations of scientists. The legacy of this long publishing tradition is an unrivalled catalogue of past publications, some of which have been unavailable from us for many years. By popular demand, Oxford University Press is now reissuing some of its most celebrated science classics in the Oxford Classic Texts series. The titles to be included have been selected not only for their historic significance, but also for their enduring eloquence and clarity of presentation. Individually, each book in this collection represents a milestone in the development of scientific thought and pedagogy; collectively these books amount to an unparalleled scientific library for the enjoyment of a new generation of readers.
Author : Kenneth R. Lang
Publisher : Springer Science & Business Media
Page : 368 pages
File Size : 49,6 Mb
Release : 2013-04-18
Category : Science
ISBN : 9783662042809
A comprehensive account of solar astrophysics and how our perception and knowledge of this star have gradually changed as mankind has elucidated ever more of its mysteries. The emphasis here is on the last decade, which has seen three successful solar spacecraft missions: SOHO, Ulysses and Yohkoh. Together, these have confirmed many aspects of the solar standard model and provided new clues to the numerous open questions that remain. The author, a leading researcher in the field, writes in a clear and concise style. Known also for his famous books "Astrophysical Formulae", "Sun, Earth and Sky" and the prize-winning "Wanderers in Space", he has succeeded once again in addressing a complex scientific topic in a very approachable way.
Author : Herbert J. Wiehl
Publisher : Unknown
Page : 120 pages
File Size : 41,7 Mb
Release : 1983
Category : Solar flares
ISBN : NASA:31769000559438
Author : Lev Dorman
Publisher : Springer Science & Business Media
Page : 912 pages
File Size : 40,8 Mb
Release : 2010-07-15
Category : Science
ISBN : 9789048137374
Short Historical Overview In the 1940s, two phenomena in the ?eld of cosmic rays (CR) forced scientists to think that the Sun is a powerful source of high-energy particles. One of these was discovered because of the daily solar variation of CR, which the maximum number of CR observed near noon (referring to the existence of continuous ?ux of CR from the direction of the Sun); this became the experimental basis of the theory that CR’s ́ originate from the Sun (or, for that matter, from within the solar system) (Alfven 1954). The second phenomenon was discovered when large ?uxes of high energy particles were detected from several solar ?ares, or solar CR. These are the - called ground level events (GLE), and were ?rst observed by ionization chambers shielded by 10 cm Pb (and detected mainly from the secondary muon-component CR that they caused) during the events of the 28th of February 1942, the 7th of March 1942, the 25th of July 1946, and the 19th of November 1949. The biggest such event was detected on the 23rd of February 1956 (see the detailed description in Chapters X and XI of Dorman, M1957). The ?rst phenomenon was investigated in detail in Dorman (M1957), by ?rst correcting experimental data on muon temperature effects and then by using coupling functions to determine the change in particle energy caused by the solar-diurnal CR variation.
Author : E.L. Chupp
Publisher : Springer Science & Business Media
Page : 332 pages
File Size : 46,6 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789401014960
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.
