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THE ELLIPTICITY CONDITION OF THE MONGE-AMPERE EQUATION IN THE SOLENOIDAL MODEL

机译:电磁模型中的安培方程的椭圆性条件

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The aim of the present paper is to discuss the influence of the ellipticity condition of the momentum divergence equation on the solution of non-divergent equation of the solenoidal or geostrophic models in the barotropic approaches. The equation considered is a nonlinear differential equation of Monge-Ampere type used for determining a streamfunction field if the geopotential field is known. It is obtained by transforming the governing equations and assuming that the divergence of wind field is equal to zero. The nonlinear balance equation is a part of the general system equations describing quasi-solenoidal or quasi-geostrophic models. Making use of the real aerological measurement data furnished by the international GRID network, the Monge-Ampere equation has been solved numerically together with the solenoidal model in barotropic approximation (a forecast for 12 hours). The results may be treated as a stage in the search for a relation between the numerical results and the processes observed in the satellite pictures. The position of the prognostic relative rotation contour line of zero (Ω = 0) may be used for determining the direction of movement of a front cloud belt.
机译:本文的目的是讨论正压方法中动量散度方程的椭圆性条件对螺线管或地转模型非散度方程解的影响。如果已知地势场,则考虑的方程是Monge-Ampere类型的非线性微分方程,用于确定流函数场。它是通过变换控制方程并假定风场的散度等于零而获得的。非线性平衡方程是描述准电磁模型或准地转模型的一般系统方程的一部分。利用国际GRID网络提供的实际航空测量数据,Monge-Ampere方程与螺线管模型正压逼近一起得到了数值求解(预测为12小时)。结果可被视为搜索数值结果与卫星图像中观察到的过程之间的关系的阶段。可预测的相对旋转轮廓线零(Ω= 0)的位置可用于确定前云带的运动方向。

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