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TEACHING EARTH SCIENCES ● Volume 26 ● Number 3, 2001<br />

Reviews<br />

An introduction to Atmospheric Physics by David G. Andrews<br />

Cambridge University Press, 2000, £17.95 (paperback), £50 (hardback).<br />

ISBN 0-521-62051-1.<br />

This book, as stated in the preface, is<br />

intended as an introductory text for<br />

third or fourth year undergraduates<br />

studying atmospheric physics, for<br />

graduate students studying atmospheric<br />

physics for the first time and for<br />

students of applied mathematics,<br />

physical chemistry and engineering who<br />

have an interest in the atmosphere. As<br />

such it assumes a basic knowledge of<br />

thermodynamics, electromagnetic<br />

radiation and quantum physics, together<br />

with some vector calculus. Its emphasis<br />

throughout is on the basic physical<br />

principles and their expression in an<br />

atmospheric context, rather than on a<br />

range of applications. Thus, it covers the<br />

three fundamental pillars of atmospheric<br />

physics – thermodynamics, radiation and<br />

fluid mechanics – with additional<br />

chapters on stratospheric chemistry,<br />

remote sensing and atmospheric<br />

modelling.<br />

The style of the book follows that of<br />

an earlier successful atmospheric physics<br />

text from an Oxford University author –<br />

Physics of Atmospheres by J. T.<br />

Houghton – in that an extensive list of<br />

problems follows each chapter which<br />

both illustrate the fundamental<br />

principles and introduce important<br />

applications. The problems will be<br />

indispensable to a serious student<br />

seeking to learn from this book and<br />

represent a valuable resource for<br />

<strong>teaching</strong> atmospheric science within<br />

physics courses. Solutions to each<br />

problem (and hints on how to obtain<br />

some of them) are provided at the end of<br />

the book.<br />

As expected from the target<br />

readership, the text concentrates on<br />

developing the basic equations of<br />

atmospheric physics from the first<br />

principles, explaining the many<br />

approximations and shortcuts that can<br />

make this branch of classical physics so<br />

confusing for undergraduates. Its remit<br />

is the <strong>Earth</strong>’s neutral atmosphere, from<br />

the ground to around 100 km altitude,<br />

which contains the weather and climate<br />

and the ozone layer as well as less<br />

familiar phenomena such as noctilucent<br />

clouds; it does not cover the ionosphere<br />

and magnetosphere.<br />

A short initial chapter introduces<br />

some essential terminology, presents the<br />

mean temperature and wind fields of the<br />

atmosphere and introduces some of the<br />

key phenomena (such as Rossby waves<br />

and the greenhouse effect) treated in<br />

detail in later chapters. This leads on to<br />

the second chapter, on atmospheric<br />

thermodynamics. The treatment here<br />

follows Houghton in introducing the<br />

tephigram – an invaluable graphical tool<br />

for representing the thermodynamic<br />

state of the troposphere, much used by<br />

meteorologists but often omitted from<br />

the basic text books. The introduction to<br />

cloud physics at the end of this chapter<br />

is rather short, and a reader interested in<br />

this subject will need to consult more<br />

specialised texts (one of which is given<br />

here as a reference).<br />

The strength of this book is<br />

the way it develops the<br />

fundamental ideas of<br />

atmospheric physics without<br />

introducing too much<br />

extraneous detail.<br />

The third chapter, on radiation, first<br />

derives basic equations of radiative<br />

transfer and spectroscopy before going<br />

on to describe the interaction of<br />

ultraviolet, visible and infrared radiation<br />

with the atmosphere. This leads on to a<br />

more detailed discussion of the<br />

greenhouse effect and atmospheric<br />

scattering. The mathematical<br />

development in this chapter is measured<br />

and carefully builds on basic principles; a<br />

careful balance must be struck between<br />

detail and clarity in this subject and<br />

Andrews is more successful than most<br />

authors in presenting this material in<br />

introductory texts.<br />

The two chapters on fluid mechanics<br />

are the best of the eight chapters in the<br />

book. They begin by deriving from first<br />

principles the basic equations of fluid<br />

dynamics, since this topic is often<br />

omitted from undergraduate physics<br />

courses. By building up carefully to<br />

quasi-geostrophic theory, gravity waves<br />

and Rossby waves the text emphasises<br />

the common principles underlying these<br />

concepts as well as opening up a broad<br />

field of atmospheric flows to quantitative<br />

study. This allows baroclimic and<br />

barotropic instability – topics often<br />

guarded by a palisade of differential<br />

equations in other texts – to be explained<br />

in a straightforward and logical way at<br />

the end of the chapter. An introduction<br />

to Ekman flow in the boundary layer is<br />

also included.<br />

The book concludes with three<br />

shorter chapters, on stratospheric<br />

chemistry, remote sounding and<br />

modelling. That on chemistry covers the<br />

basic concepts of atmospheric chemistry<br />

and provides an introduction to the<br />

Antarctic ozone hole. The remote<br />

sounding chapter has an impressive<br />

breadth for a book of this type, covering<br />

both passive and active (radar, lidar)<br />

ground-based methods as well as the<br />

more conventional space observations.<br />

The short final chapter gives a brief<br />

introduction to atmospheric modelling.<br />

The strength of this book is the way it<br />

develops the fundamental ideas of<br />

atmospheric physics without introducing<br />

too much extraneous detail. Its level is<br />

very well suited to its target readership<br />

and it is considerably more affordable<br />

than some of its competitors. Thus, I<br />

expect this book to become a standard<br />

text for many atmospheric physics<br />

courses in future years.<br />

Geraint Vaughan<br />

Department of Physics<br />

University of Wales Aberystwyth<br />

www.esta-uk.org<br />

116

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