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"The solar atmosphere above the photosphere, the Sun's surface layers, is heated up to Mega-kelvin temperatures and raised to a high level of dynamic activity through processes involving a pervading magnetic field. This book is concerned with one of the most important means of understanding the solar atmosphere, its ultraviolet and soft X-ray emission. The ultraviolet and X-ray spectra of the Sun's atmosphere provide valuable information about its nature - the heat and density of its various parts, its dynamics, and its chemical composition." "Spacecraft instrumentation from Skylab, the P78-1 mission, SolarMax, Yohkoh, Soho, Trace, and Hinode are described. With introductions to atomic physics and the diagnostic techniques used by solar spectroscopists, a list of emission lines in the ultraviolet and soft X-ray region, and a glossary of terms, this book is an ideal reference for graduate students and researchers in astrophysics and solar physics."--Jacket.
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1
Ultraviolet and X-Ray Spectroscopy of the Solar Atmosphere
2012, University of Cambridge ESOL Examinations
in English
1107407915 9781107407916
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2
Ultraviolet and X-Ray Spectroscopy of the Solar Atmosphere
2011, Cambridge University Press
in English
051141076X 9780511410765
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3
Ultraviolet and X-Ray Spectroscopy of the Solar Atmosphere
2009, Cambridge University Press
in English
0511585969 9780511585968
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4
Ultraviolet and x-ray spectroscopy of the solar atmosphere
2008, Cambridge University Press
in English
0521841607 9780521841603
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Includes bibliographical references and index.
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