Leon Golub, Harvard-Smithsonian Center for Astrophysics, Jay M. Pasachoff, Williams College
EDITION STATEMENT
Edition Statement
Second edition
PHYSICAL DESCRIPTION
Specific Material Designation and Extent of Item
xvi, 297 pages :
Other Physical Details
illustrations (some color) ;
Dimensions
24 cm
INTERNAL BIBLIOGRAPHIES/INDEXES NOTE
Text of Note
Includes bibliographical references and index
CONTENTS NOTE
Text of Note
The sun -- The once and future sun -- What we see : the solar disk -- What we don't see -- Eclipses -- Space missions -- Between fire and ice -- Space weather
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SUMMARY OR ABSTRACT
Text of Note
"How did the Sun evolve, and what will it become? What is the origin of its light and heat? How does solar activity affect the atmospheric conditions that make life on Earth possible? These are the questions at the heart of solar physics, and at the core of this book. The Sun is the only star near enough to study in sufficient detail to provide rigorous tests of our theories and to help us understand the more distant and exotic objects throughout the cosmos. Having observed the Sun using both ground-based and spaceborne instruments, the authors bring their extensive personal experience to this story revealing what we have discovered about phenomena from eclipses to neutrinos, space weather, and global warming. This Second Edition is updated throughout, and features results from the current spacecraft that are aloft, especially NASA's Solar Dynamics Observatory, for which one of the authors designed some the telescopes"--Provided by publisher