Nuclear processes in the solar atmosphere and the particle-acceleration problem
Author: R. A. Syunyaev
Publisher: CRC Press
Published: 1988
Total Pages: 124
ISBN-13: 9783718648405
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Author: R. A. Syunyaev
Publisher: CRC Press
Published: 1988
Total Pages: 124
ISBN-13: 9783718648405
DOWNLOAD EBOOKAuthor: Charles Philip Sonett
Publisher: University of Arizona Press
Published: 1991
Total Pages: 1040
ISBN-13: 9780816512973
DOWNLOAD EBOOKAn interdisciplinary approach to solar physics, as eighty-nine contributors trace the evolution of the Sun and provide a review of our current understanding of both its structure and its role in the origin and evolution of the solar system.
Author: L.I. Miroshnichenko
Publisher: Springer Science & Business Media
Published: 2013-06-29
Total Pages: 489
ISBN-13: 9401596468
DOWNLOAD EBOOKIt turned out to be really a rare and happy occasion that we know exact1y when and how a new branch of space physics was born, namely, a physics of solar cosmic rays. It happened on February 28 and March 7, 1942 when the fIrst "cosmic ray bursts" were recorded on the Earth, and the Sun was unambiguously identifIed for the fIrst time as the source of high-velocity 10 particles with energies up to > 10 eV. Just due to such a high energy these relativistic particles have been called "solar cosmic rays" (SCR), in distinction from the "true" cosmic rays of galactic origin. Between 1942 and the beginning ofthe space era in 1957 only extremely high energy solar particle events could be occasionally recorded by cosmic ray ground-Ievel detectors and balloon borne sensors. Since then the detection techniques varied considerably and the study of SCR turned into essential part of solar and solar-terrestrial physics.
Author: U. Esser
Publisher: Springer Science & Business Media
Published: 2013-11-11
Total Pages: 1110
ISBN-13: 3662123614
DOWNLOAD EBOOKAstronomy and Astrophysics Abstracts aims to present a comprehensive documen tation of the literature concerning all aspects of astronomy, astrophysies, and their border fields. It is devoted to the recording, summarizing, and indexing of the relevant publications throughout the world. Astronomy and Astrophysics Abstracts is prepared by a special department of the Astronomisches Rechen-Institut under the auspices of the International Astronomical Union. Volume 44 records literature published in 1987 and received before February 15, 1988. Some older documents which we received late and which are not surveyed in earlier volumes are inc1uded too. We acknowledge with thanks contributions of our colleagues all over the world. We also express our gratitude to all organiza tions, observatories, and publishers which provide us with complimentary copies of their publications. Dr. Siegfried Böhme retired from his duties as co-editor of Astronomy and Astro physics Abstracts on December 31, 1987. Since 1950 he partieipated in the biblio graphie work of the institute. He served as a reviewer for the Astronomischer Jahresbericht and became one of the editors of Astronomy and Astrophysics Ab stracts in 1969. After his retirement in 1975 he took care of, particularly, the Russian literature on a voluntary basis for 12 years. It is a pleasure to thank Siegfried Böhme for his valuable contributions. Starting with Volume 33, all the recording, correction, and data processing work was done by means of computers. The recording was done by our technical staff members Ms. Helga Ballmann, Ms. Christiane Jehn, Ms. Monika Kohl, Ms.
Author: Leonty Miroshnichenko
Publisher: Springer
Published: 2014-10-16
Total Pages: 533
ISBN-13: 3319094297
DOWNLOAD EBOOKPresents a comprehensive approach to the open questions in solar cosmic ray research and includes consistent and detailed considerations of conceptual, observational, theoretical, experimental and applied aspects of the field. The results of solar cosmic ray (SCR) investigations from 1942 to the present are summarized in this book. It treats the research questions in a self-contained form in all of its associations, from fundamental astrophysical aspects to geophysical, aeronautical and cosmonautical applications. A large amount of new data is included, which has been accumulated during the last several decades of space research. This second edition contains numerous updates and corrections to the text, figures and references. The author has also added several new sections about GLEs and radiation hazards. In addition, an extensive bibliography is provided, which covers non-partially the main achievements and failures in the field. This volume is aimed at graduate students and researchers in solar physics and space science.
Author: R. A. Syunyaev
Publisher: CRC Press
Published: 1988
Total Pages: 104
ISBN-13: 9783718648382
DOWNLOAD EBOOKAuthor: Yu. N. Efremov
Publisher: CRC Press
Published: 1989
Total Pages: 88
ISBN-13: 9783718649266
DOWNLOAD EBOOKDescribed is the contribution of the comets in the Oort cloud to the angular momentum of the solar system.
Author: R. A. Syunyaev
Publisher: CRC Press
Published: 1988
Total Pages: 132
ISBN-13: 9783718648399
DOWNLOAD EBOOKContains two reviews of astrophysical interest: Supernovae and Supernova Remnants, and Observations of Cosmic Gamma-Ray Bursts. (NW) Annotation copyrighted by Book News, Inc., Portland, OR
Author: D. G. Yakovlev
Publisher: CRC Press
Published: 1989
Total Pages: 88
ISBN-13: 9783718649242
DOWNLOAD EBOOKAuthor: B.V. Somov
Publisher: Springer Science & Business Media
Published: 2012-12-06
Total Pages: 255
ISBN-13: 9401123969
DOWNLOAD EBOOKSolar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of techniques from Earth and from space. The aim is to discover the physics behind solar flares. This goal is complicated because information about the flare mechanism can be obtained only in an indirect way by studying the secondary effects. This book provides three stages in the solution of the solar flare problem. Chapter one describes the connection between observational data and theoretical concepts, where it is stressed that next to investigating flares, the related non-stationary large-scale phenomena must be studied as well. The second chapter deals with secondary physical processes, in particular the study of high-temperature plasma dynamics during impulsive heating. The last chapter presents a model built on the knowledge of the two previous chapters and it constructs a theory of non-neutral turbulent current sheets. The author believes that this model will help to solve the problem of solar flares. For solar physicists, plasma physicists, high-energy particle physicists.