Physics Of The Solar Corona PDF Download
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Author | : Markus Aschwanden |
Publisher | : Springer Science & Business Media |
Total Pages | : 946 |
Release | : 2006-01-30 |
Genre | : Science |
ISBN | : 9783540307655 |
Download Physics of the Solar Corona Book in PDF, ePub and Kindle
A thorough introduction to solar physics based on recent spacecraft observations. The author introduces the solar corona and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, together with their potential effects on the Earth.
Author | : I. S. Shklovskii |
Publisher | : Pergamon |
Total Pages | : 575 |
Release | : 1965 |
Genre | : Sun |
ISBN | : 9780080137520 |
Download Physics of the Solar Corona Book in PDF, ePub and Kindle
Author | : Leon Golub |
Publisher | : Cambridge University Press |
Total Pages | : 405 |
Release | : 2010 |
Genre | : Science |
ISBN | : 052188201X |
Download The Solar Corona Book in PDF, ePub and Kindle
Second edition graduate level textbook giving an up-to-date treatment of our understanding of the solar corona.
Author | : C.J. Macris |
Publisher | : Springer |
Total Pages | : 370 |
Release | : 1971-12-31 |
Genre | : Science |
ISBN | : |
Download Physics of the Solar Corona Book in PDF, ePub and Kindle
Proceedings of the NATO Advanced Institute on Physics of the Solar Corona, held in Cavouri-Vouliagmeni, Athens, Greece, 6-17 September 1970
Author | : Markus Aschwanden |
Publisher | : Springer |
Total Pages | : 908 |
Release | : 2006-08-26 |
Genre | : Science |
ISBN | : 9783540307662 |
Download Physics of the Solar Corona Book in PDF, ePub and Kindle
A thorough introduction to solar physics based on recent spacecraft observations. The author introduces the solar corona and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, together with their potential effects on the Earth.
Author | : Oddbjorn Engvold |
Publisher | : Springer Science & Business Media |
Total Pages | : 492 |
Release | : 2013-03-09 |
Genre | : Science |
ISBN | : 9401734291 |
Download The Physics of the Solar Corona and Transition Region Book in PDF, ePub and Kindle
Solar Physics publishes up to two Topical Issues per year that focus on areas of especially vigorous and active research. The present Topical Issue contains papers of recent results on the solar corona, as well as on the transition region and low solar wind. The majority of these papers, which were all refereed in accordance with the standards of Solar Physics, were presented in August 1999 at a workshop held in Monterey, California. The authors were offered the opportunity to present relevant parts of their contributions on an accompanying CD ROM of this Topical Issue. The Sun's magnetic field is responsible for the spectacularly dynamic and intri cate phenomenon that we call the corona. The past decade has seen an enormous increase in our understanding of this part of the solar outer atmosphere, both as a result of observations and because of rapid advances in numerical studies. The Yohkoh satellite has observed the Sun now for over eight years, producing spectac ular sequences of images that convey the complexity of the corona. The imaging and spectroscopic instruments on SOHO have added information on the cooler part of the corona. And since April of 1998 TRACE has given us very high resolution images of the 1-2 MK corona, at cadences that allow detailed observations of field oscillations, loop evolution, mass ejecta, etc.
Author | : R.G. Athay |
Publisher | : Springer Science & Business Media |
Total Pages | : 517 |
Release | : 2012-12-06 |
Genre | : Science |
ISBN | : 9401017158 |
Download The Solar Chromosphere and Corona: Quiet Sun Book in PDF, ePub and Kindle
The widespread tendency in solar physics to divide the solar atmosphere into separate layers and to distinguish phenomena of solar activity from phenomena of the quiet Sun emphasizes the wide ranging diversity of physical conditions and events occurring in the solar atmosphere. This diversity spans the range from a neutral, essentially quiescent atmosphere to a highly ionized, violently convective atmosphere; from a domain in which magnetic field effects are unimportant to a domain in which the magnetic pressure exceeds the gas pressure, and from a domain in which the particle motions are Maxwellian to a domain in which an appreciable fraction of the particles is accelerated to relativistic energies. It is now widely recognized that the chromosphere and corona have a common origin in the mechanical energy flux generated in the hydrogen convection zone lying beneath the photosphere. Furthermore, magnetic field phenomena appear to be as vital to the structure of th~ quiet Sun as to the active Sun. For these reasons it appears desirable to present a unified treatment of the entire solar atmosphere, both active and quiet, in a single volume. On the other hand, such a treatise must be very long if it is to avoid being superficial, and it is very difficult for a single author to write authoritatively on such a wide range of topics.
Author | : Oddbjorn Engvold |
Publisher | : Springer Science & Business Media |
Total Pages | : 402 |
Release | : 2012-12-06 |
Genre | : Science |
ISBN | : 9401008604 |
Download Physics of the Solar Corona and Transition Region Book in PDF, ePub and Kindle
Proceedings of the Monterey Workshop, held in Monterey, California, August 1999
Author | : I. S. Shklovskiĭ |
Publisher | : |
Total Pages | : 496 |
Release | : 1965 |
Genre | : Sun |
ISBN | : |
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Author | : A. J. Hundhausen |
Publisher | : Springer Science & Business Media |
Total Pages | : 250 |
Release | : 2012-12-06 |
Genre | : Science |
ISBN | : 3642654142 |
Download Coronal Expansion and Solar Wind Book in PDF, ePub and Kindle
Little more than ten years have passed since spaceprobe-borne instruments con clusively demonstrated the existence of the solar wind. These observations con firmed the basic validity of a theoretical model, first proposed by E. N. Parker, predicting a continuous, rapid expansion of the solar corona. The subsequent decade has seen a tremendous growth in both the breadth and sophistication of solar wind observations; the properties of the interplanetary plasma near the orbit of the earth are now known in great detail. The theory of the coronal ex pansion has also been highly refilled both in the sense of including additional physical processes, and of treating more realistic (time-dependent and non spheri cally-symmetric) coronal boundary conditions. The present volume is an attempt to synthesize the solar wind observations and coronal expansion models from this decade of rapid development. The ultimate goal is, of course, the interpretation of observed solar wind phenomena as the effects of basic physical processes occurring in the coronal and interplanetary plasma and as the natural manifestations of solar properties and structures. This approach implies an emphasis upon the "large-scale" features revealed by the observations. It requires extensive use of the concepts and methods of fluid mechanics.