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ISBN
:
9780521382618
Publisher
:
Cambridge University Press
Subject
:
Astronomy, Space & Time, Physics
Binding
:
HARDCOVER
Pages
:
290
Year
:
1993
₹
8104.0
₹
6402.0
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The solar transition region that spans the temperature range from about 20,000 to 1,000,000 K separates the solar chromosphere from the corona. All energy that heats the corona and powers the solar wind must pass through this part of the solar atmosphere. This book summarizes recent ultraviolet and extreme ultraviolet observations of the transition region, the empirical models derived from them, and the physical models that try to explain both the observations and the empirical models. The observational focus is on quiet solar transition region observations made with Skylab and subsequent rocket and satellite experiments. The book also presents a unified discussion of the analysis of ultraviolet and extreme ultraviolet spectroscopic data including the determination of the emission measure and density and temperature diagnostics. This will be usefulto astrophysicists who are confronting high-resolution ultraviolet and extreme ultraviolet data from astrophysical plasmas for the first time.
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