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TOPICS IN GEOPHYSICAL FLUID DYNAMICS: ATMOSPHERIC By M. Ghil & S. Childress *VG*

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Specifiche dell'oggetto

Condizione
Ottime condizioni: Libro che non sembra nuovo ed è già stato letto, ma è in condizioni eccellenti. ...
Book Title
Topics in Geophysical Fluid Dynamics: Atmospheric Dynamics,
Item Height
9.25 inches
ISBN-10
0387964754
ISBN
9780387964751

Informazioni su questo prodotto

Product Identifiers

Publisher
Springer New York
ISBN-10
0387964754
ISBN-13
9780387964751
eBay Product ID (ePID)
139720

Product Key Features

Number of Pages
Xv, 512 Pages
Publication Name
Topics in Geophysical Fluid Dynamics : Atmospheric Dynamics, Dynamo Theory, and Climate Dynamics
Language
English
Publication Year
1987
Subject
Earth Sciences / Meteorology & Climatology, Physics / Mathematical & Computational
Type
Textbook
Subject Area
Science
Author
M. Ghil, S. Childress
Series
Applied Mathematical Sciences Ser.
Format
Trade Paperback

Dimensions

Item Weight
55.4 Oz
Item Length
9.3 in
Item Width
6.1 in

Additional Product Features

Intended Audience
Scholarly & Professional
LCCN
86-031387
Dewey Edition
19
Series Volume Number
60
Number of Volumes
1 vol.
Illustrated
Yes
Dewey Decimal
510 s
Table Of Content
I. Fundamentals.- 1. Effects of Rotation.- 2. Effects of Shallowness.- 3. The Quase-Geostrophic Approximation.- II. Large-Scale Atmospheric Dynamics.- 4. Effects of Stratification Baroclinic Instability.- 5. Changing Flow Patterns and Successive Bifurcations.- 6. Persistent Anomalies, Blocking and Predictability.- III. Dynamo Theory.- 7. Models of Geomagnetism: A Survey.- 8. Kinematic Dynamo Theory.- 9. The Hydrodynamic Basis of Geomagnetism.- IV. Theoretical Climate Dynamics.- 10. Radiation Balance and Equilibrium Models.- 11. Glaciation Cycles: Phenomenology and Slow Processes.- 12. Climatic Oscillators.- References.
Synopsis
The vigorous stirring of a cup of tea gives rise, as we all know, to interesting fluid dynamical phenomena, some of which are very hard to explain. In this book our "cup of tea" contains the currents of the Earth's atmosphere, oceans, mantle, and fluid core. Our goal is to under- stand the basic physical processes which are most important in describing what we observe, directly or indirectly, in these complex systems. While in many respects our understanding is measured by the ability to predict, the focus here will be on relatively simple models which can aid our physical intuition by suggesting useful mathematical methods of investiga- tion. These elementary models can be viewed as part of a hierarchy of models of increasing complexity, moving toward those which might be use- fully predictive. The discussion in this book will deal primarily with the Earth. Interplanetary probes of Venus, Mars, Jupiter and Saturn have revealed many exciting phenomena which bear on geophysical fluid dynamics. They have also enabled us to see the effect of changing the values of certain parameters, such as gravity and rotation rate, on geophysical flows. On the other hand, satellite observations of our own planet on a daily and hourly basis have turned it into a unique laboratory for the study of fluid motions on a scale never dreamt of before: the motion of cyclones can be observed via satellite just as wing tip vortices are studied in a wind tunnel., The vigorous stirring of a cup of tea gives rise, as we all know, to interesting fluid dynamical phenomena, some of which are very hard to explain. In this book our "cup of tea" contains the currents of the Earth's atmosphere, oceans, mantle, and fluid core. Our goal is to under­ stand the basic physical processes which are most important in describing what we observe, directly or indirectly, in these complex systems. While in many respects our understanding is measured by the ability to predict, the focus here will be on relatively simple models which can aid our physical intuition by suggesting useful mathematical methods of investiga­ tion. These elementary models can be viewed as part of a hierarchy of models of increasing complexity, moving toward those which might be use­ fully predictive. The discussion in this book will deal primarily with the Earth. Interplanetary probes of Venus, Mars, Jupiter and Saturn have revealed many exciting phenomena which bear on geophysical fluid dynamics. They have also enabled us to see the effect of changing the values of certain parameters, such as gravity and rotation rate, on geophysical flows. On the other hand, satellite observations of our own planet on a daily and hourly basis have turned it into a unique laboratory for the study of fluid motions on a scale never dreamt of before: the motion of cyclones can be observed via satellite just as wing tip vortices are studied in a wind tunnel.
LC Classification Number
QC19.2-20.85

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