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Adaptivity with moving grids

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92 C. J. Budd, W. Huang and R. D. Russell<br />

solving nonlinear PDEs which can often be naturally modified for <strong>moving</strong><br />

mesh algorithms, in such a way that the discrete solutions share common<br />

properties <strong>with</strong> the (unknown) analytical solutions; and to show that the<br />

sharing of the common structures leads to efficient adaptive methods.<br />

5.1. Symmetry, self-similar solutions and scale invariance<br />

Many naturally occurring physical systems have an invariance under symmetries<br />

including translations, rotations and changes of scale, and this is<br />

reflected in the partial differential equations that describe them. The solutions<br />

of these equations may then either be themselves invariant under<br />

(combinations of) these symmetries, the self-similar solutions, or they can<br />

be transformed into other solutions through the application of symmetry<br />

operators. Conservation laws can be linked through Noether’s theorem<br />

(Olver 1986, Dorodnitsyn 1993b) to many of the continuous symmetries.<br />

An example of such a system is Burgers’ equation,<br />

u t + u · ∇u = ν∆u,<br />

which is invariant under rotations in space and translations in both space<br />

and time. It admits travelling-wave solutions which are self-similar solutions<br />

coupling spatial and temporal translation, <strong>with</strong> the wave speed giving the<br />

coupling. The waves can be at any orientation, and the action of a rotation<br />

is to map one wave to another. In other systems a rescaling of space, time<br />

and of the solution leaves the partial differential equations governing the<br />

system invariant. Such changes of scale were first observed by Kepler in<br />

his studies of the solar system and summarized in his famous third law, in<br />

which he observed that if a planetary orbit existed <strong>with</strong> a solution (in polar<br />

coordinates) given by (r(t),θ(t)) then there was also a solution of the form<br />

(<br />

(λ 3 r(λ 2 t)), O(λ 2 t) ) for any positive value of λ. Such scaling invariance also<br />

arises in the equations of fluid and gas dynamics, nonlinear optics and many<br />

biological systems. An excellent summary of scale-invariant systems <strong>with</strong><br />

such properties is given in the book by Barenblatt (1996).<br />

We can then ask the question of whether a numerical method can be<br />

constructed which is also invariant under symmetries. More generally, an<br />

adaptive method can be designed to exploit the symmetries in the problem.<br />

In a sense, the answer to this question is obvious as we can always perform<br />

an aprioriscaling of the problem and then use a method in the scaled<br />

coordinates. However, this assumes more knowledge of the physical system<br />

than we may easily have available to us. Indeed, for some systems there<br />

are a number of different possible changes of scale, and it is not apriori<br />

obvious which one correctly describes the system evolution.<br />

We now show how several of the <strong>moving</strong> mesh strategies described earlier,<br />

particularly those based on <strong>moving</strong> mesh partial differential equations, can<br />

be very effectively applied to such problems <strong>with</strong> symmetry. Such methods

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