Introduction to Modeling Convection in Planets and Stars – Magnetic Field, Density Stratification, Rotation: 24 (Princeton Series in Astrophysics) - Image 1

£70.22

Princeton University Press Introduction to Modeling Convection in Planets and Stars – Magnetic Field, Density Stratification, Rotation: 24 (Princeton Series in Astrophysics)

Name: Introduction to Modeling Convection in Planets and Stars - Magnetic Field, Density Stratification, Rotation: 24 (Princeton Series in Astrophysics)
Brand: Princeton University Press
Price: 70.22 GBP
Availability: InStock

Theoretical & Mathematical Astronomy

It has never been this cheap. We have no record of a lower price.

£70 today · cheaper than every other day in the last 3 months

NEW HERE?

Amazon shows you one price. We show you all of them.

Tosheroon watches Amazon prices so you don't have to. Every product on Amazon has a price history — we make it visible. Set the price you'd actually pay, and we'll email you the second it gets there. No app, no account, one email.

WHAT'S ON THIS PAGE

↓ Price chart
when this has been cheap or pricey

↓ Forecast
where the price is heading next

↓ Statistics
all-time high & low, recent range

↑ Price alert
name your number, we'll email you

Price History & Forecast

Grey patches = out of stock. Cheaper = lower on the chart. Hover for exact prices.

Last 70 days • 70 data points (No recent data available)

Historical

Generating forecast...

Price Distribution

Price distribution over 70 days • 1 price levels

Days at Price

Price Analysis

Most common price: £70 (70 days, 100.0%)

Price range: £70 - £70

Price levels: 1 different prices over 70 days

Description

This book provides readers with the skills they need to write computer codes that simulate convection, internal gravity waves, and magnetic field generation in the interiors and atmospheres of rotating planets and stars. Using a teaching method perfected in the classroom, Gary Glatzmaier begins by offering a step-by-step guide on how to design codes for simulating nonlinear time-dependent thermal convection in a two-dimensional box using Fourier expansions in the horizontal direction and finite differences in the vertical direction. He then describes how to implement more efficient and accurate numerical methods and more realistic geometries in two and three dimensions. In the third part of the book, Glatzmaier demonstrates how to incorporate more sophisticated physics, including the effects of magnetic field, density stratification, and rotation. Featuring numerous exercises throughout, this is an ideal textbook for students and an essential resource for researchers. * Describes how to create codes that simulate the internal dynamics of planets and stars * Builds on basic concepts and simple methods * Shows how to improve the efficiency and accuracy of the numerical methods * Describes more relevant geometries and boundary conditions * Demonstrates how to incorporate more sophisticated physics

Product Specifications

Brand: Princeton University Press
Format: hardcover
ASIN: 069114172X
Category: Books > Subjects > Science, Nature & Maths > Astronomy & Space Science > Astronomy > Theoretical & Mathematical Astronomy
Domain: Amazon UK
Release Date: 04 December 2013
Listed Since: 14 October 2008

Barcode

No barcode data available

Princeton University Press Introduction to Modeling Convection in Planets and Stars – Magnetic Field, Density Stratification, Rotation: 24 (Princeton Series in Astrophysics)

It has never been this cheap. We have no record of a lower price.

Price History & Forecast

Price Distribution

Price Analysis

Description

Product Specifications

Barcode

Similar Products You Might Like

Introduction to Modeling Convection in Planets and Stars: Magnetic Field, Density Stratification, Rotation (Princeton Series in Astrophysics): 24

Multi-scale Dynamical Processes in Space and Astrophysical Plasmas: 33 (Astrophysics and Space Science Proceedings, 33)

Multi-scale Dynamical Processes in Space and Astrophysical Plasmas: 33 (Astrophysics and Space Science Proceedings, 33)

Theory of Rotating Stars. (PSA-1) (Princeton Series in Astrophysics): 27 (Princeton Legacy Library)

Astrophysical Data: Planets and Stars

Fluid Dynamics and Dynamos in Astrophysics and Geophysics: 12 (The Fluid Mechanics of Astrophysics and Geophysics)

Interpreting Astronomical Spectra

Mathematical Aspects of Natural Dynamos (The Fluid Mechanics of Astrophysics and Geophysics)

Planetary Science: The Science of Planets around Stars, Second Edition

Solar and Stellar Magnetic Fields (IAU S354): Origins and Manifestations (Proceedings of the International Astronomical Union Symposia and Colloquia)

Theory of Stellar Atmospheres: An Introduction to Astrophysical Non-equilibrium Quantitative Spectroscopic Analysis (Princeton Series in Astrophysics): 26

Theory of Stellar Atmospheres – An Introduction of Astrophysical Non–equilibrium Quantitative Spectroscopic Analysis: An Introduction to ... Analysis (Princeton Series in Astrophysics)

The Physics of the Interstellar Medium

Stellar Atmospheres: Beyond Classical Models: 341 (Nato Science Series C:, 341)

The Numerical Modelling of Nonlinear Stellar Pulsations: Problems and Prospects: 302 (Nato Science Series C:, 302)

The Numerical Modelling of Nonlinear Stellar Pulsations: Problems and Prospects: 302 (Nato Science Series C:, 302)

Numerical Methods in Astrophysics: An Introduction (Series in Astronomy and Astrophysics)

Radial-velocity Searches for Planets Around Active Stars (Springer Theses)

Turbulence and Magnetic Fields in Astrophysics: 614 (Lecture Notes in Physics, 614)

Numerical Python in Astronomy and Astrophysics: A Practical Guide to Astrophysical Problem Solving (Undergraduate Lecture Notes in Physics)

Magnetodynamic Phenomena in the Solar Atmosphere: Prototypes of Stellar Magnetic Activity

Planetary Science: The Science of Planets around Stars, Second Edition

ВИХРОВА ТЕОРІЯ УТВОРЕННЯ І ЕВОЛЮЦІЇ ПЛАНЕТНИХ І ГАЛАКТИЧНИХ СИСТЕМ

Astrochemical Modeling: Practical Aspects of Microphysics in Numerical Simulations