2016
DOI: 10.1007/s40430-016-0678-4
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A space–time CESE scheme for shallow water magnetohydrodynamics equations with variable bottom topography

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Cited by 3 publications
(2 citation statements)
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“…The consideration of the shallow water equations in the presence of a magnetic field (SMHD) is a relatively new area of magnetohydrodynamics. One of the first models to describe SMHD was presented in [1] (the Gilman model), and since then, many papers by various authors have been devoted to studying this model, including its stability [2], numerical simulation [3][4][5][6][7][8], and conservation laws [9,10] (see, for example, a more detailed review in [9]).…”
Section: Introductionmentioning
confidence: 99%
“…The consideration of the shallow water equations in the presence of a magnetic field (SMHD) is a relatively new area of magnetohydrodynamics. One of the first models to describe SMHD was presented in [1] (the Gilman model), and since then, many papers by various authors have been devoted to studying this model, including its stability [2], numerical simulation [3][4][5][6][7][8], and conservation laws [9,10] (see, for example, a more detailed review in [9]).…”
Section: Introductionmentioning
confidence: 99%
“…The consideration of the shallow water equations in the presence of a magnetic field (SMHD) is a relatively new area of magnetohydrodynamics. One of the first models to describe SMHD was presented in [1] (the Gilman model), and since then, many papers by various authors have been devoted to studying this model, including its stability [2], numerical simulation [3][4][5][6][7], and conservation laws [8,9] (see, for example, a more detailed review in [8]).…”
Section: Introductionmentioning
confidence: 99%