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Generalized solutions and hydrostatic approximation of the Euler equations

机译:欧拉方程的广义解和流体静力学近似

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摘要

Solutions to the Euler equations on a 3D domain D-3 (typically the unit cube or the periodic unit cube) can be formally obtained by minimizing the action of an incompressible fluid moving inside D-3 between two given configurations. When these two configurations are very close to each other, classical solutions do exist, as shown by Ebin and Marsden. However, Shnirelman found a class of data (essentially 2D in the sense that they trivially depend on the vertical coordinate) for which there cannot be any classical minimizer. For such data, generalized solutions can be shown to exist, as a substitute for classical solutions. These generalized solutions have unusual features that look highly unphysical (in particular, different fluid parcels can cross at the same point and at the same time), but the pressure field, which does not depend on the vertical coordinate, is well and uniquely defined. In the present paper. we show that these generalized solutions are actually quite conventional in the sense they obey, up to a suitable change of variable, a well-known variant (widely used for geophysical flows) of the 3D Euler equations. for which the vertical acceleration is neglected according to the so-called hydrostatic approximation.
机译:通过最小化在两个给定配置之间在D-3内部移动的不可压缩流体的作用,可以正式获得3D域D-3(通常是单位立方或周期性单位立方)上的Euler方程的解。当这两种配置彼此非常接近时,确实存在经典解决方案,如Ebin和Marsden所示。但是,Shnirelman发现了一类数据(从某种意义上说,二维基本上取决于垂直坐标),因此没有任何经典的最小化器。对于此类数据,可以证明存在通用解决方案,以替代经典解决方案。这些广义的解决方案具有看起来非常不自然的异常特征(特别是不同的流体块可以在同一点同时穿越),但是不依赖于垂直坐标的压力场被很好地定义。在本文中。我们显示出,从广义上讲,这些广义解在遵循它们的意义上是非常常规的,直到变量发生适当的变化为止,这是3D欧拉方程的一个著名变体(广泛用于地球物理流)。对于这种情况,根据所谓的静液压近似忽略了垂直加速度。

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