Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere Cambridge Astrophysics
Hardcover. 360 pages. Dimensions: 9.8in. x 6.8in. x 0.9in.The solar atmosphere, above the Suns surface layers, reaches mega-kelvin temperatures and high levels of dynamic activity through processes involving a pervading magnetic field. This book explores one of the principal means of understanding the solar atmosphere, its ultraviolet and soft X-ray emission. The ultraviolet and X-ray spectra of the Suns atmosphere provide valuable information about its nature - the heat and density of its various parts, its dynamics, and chemical composition. The principles governing spectral line and continuous emission, and how spectral studies lead to deductions about physical properties, are described, together with spacecraft instrumentation from Skylab, SolarMax, Yohkoh, SOHO, TRACE, and Hinode. With introductions to atomic physics and diagnostic techniques used by solar spectroscopists, a list of emission lines in ultraviolet and soft X-ray regions, and a glossary of terms, this is an ideal reference for graduate students and researchers in astrophysics and solar physics. This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN. Bookseller Inventory # 9780521841603
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Book Description: Exploring a principal means of understanding the Sun's atmosphere, its ultraviolet and soft X-ray emission, this 2008 book includes a list of emission lines in the ultraviolet and soft X-ray region, and a glossary of terms. An ideal reference for graduate students and researchers in astrophysics and solar physics.
Title: Ultraviolet and X-ray Spectroscopy of the ...
Publisher: Cambridge University Press
Book Condition: New
Book Type: Hardcover
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