
A complete revision of Goody's classic 1964 work, this volume offers a systematic discussion of atmospheric radiation processes that today are at the center of worldwide study and concern. It deals with the ways in which incident solar radiation is transformed into scattered and thermal radiation, and the thermodynamic consequences for the Earth's gaseous envelope, identifying aspects of the interaction between radiation and atmospheric motions as the central theme for atmospheric radiation studies. As a complete treatment of physical and mathematical foundations, the text assumes no prior knowledge of atmospheric physics. The theoretical discussion is systematic, and can therefore be applied with minor extension to any planetary atmosphere.
This volume investigates the fundamental physical and mathematical principles governing atmospheric radiation processes and their thermodynamic impact on planetary atmospheres. R. M. Goody and Y. L. Yung provide a comprehensive framework that updates the 1964 classic, focusing on the transformation of solar radiation into scattered and thermal energy. The authors utilize a systematic approach to explain the interaction between radiation and atmospheric motion, establishing a rigorous basis for modern climate and meteorological research.
What You Will Find
Experts recognize this volume as a foundational text for students and researchers in atmospheric physics. Readers frequently note the high level of mathematical rigor and the systematic clarity that makes the complex subject matter accessible to those without prior specialized knowledge in the field.
Page Count:
540
Publication Date:
1995-01-01
Publisher:
Oxford University Press
ISBN-10:
0195356101
ISBN-13:
9780195356106
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