2009
DOI: 10.1017/cbo9780511809101
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Introduction to Numerical Geodynamic Modelling

Abstract: Numerical modelling of geodynamic processes was predominantly the domain of high-level mathematicians experienced in numerical and computational techniques. Now, for the first time, students and new researchers in the Earth Sciences can learn the basic theory and applications from a single, accessible reference text. Assuming only minimal prerequisite mathematical training (simple linear algebra and derivatives) the author provides a solid grounding in basic mathematical theory and techniques, including contin… Show more

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Cited by 285 publications
(410 citation statements)
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References 342 publications
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“…The models are solved using I3ELVIS code; it is based on the numerical solution of mass, momentum and energy conservation equations using finite difference method and marker-in cell techniques combined with a multigrid solver 23,24 . The staggered grid for which equations are solved includes 501 Â 165 Â 101 nodes with 100 million randomly distributed markers.…”
Section: Methodsmentioning
confidence: 99%
“…The models are solved using I3ELVIS code; it is based on the numerical solution of mass, momentum and energy conservation equations using finite difference method and marker-in cell techniques combined with a multigrid solver 23,24 . The staggered grid for which equations are solved includes 501 Â 165 Â 101 nodes with 100 million randomly distributed markers.…”
Section: Methodsmentioning
confidence: 99%
“…Our simulations were carried out using SiStER (Simple Stokes solver with Exotic Rheologies), a 2-D finite-difference/particle-incell code (Harlow & Welch 1965;Gerya & Yuen 2003 written in MATLAB R , and based on the methodology of Gerya (2010a). This code relies heavily on MATLAB (built-in) functions and capabilities for vector operations, and achieves computation speeds on par with standard serial compiled language codes.…”
Section: Numerical Methodologymentioning
confidence: 99%
“…Repeated indices imply summation and the first term in eq. (3) is the material time-derivative of T. These equations are discretized on an Eulerian (non-deforming) grid using a conservative finite difference scheme on a fully staggered grid (Gerya 2010a;Duretz et al 2011). The matrix equation for the discretization is defined in terms of the two velocity components and pressure, and then solved using the direct 'backslash' solver in MATLAB.…”
Section: Numerical Methodologymentioning
confidence: 99%
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