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Particle Simulations of Planetary Probe Flows Employing Automated Mesh Refinement

机译:采用自动网格细化的行星探针流的粒子模拟

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摘要

The data structures and algorithms of a newly developed three-dimensional direct simulation Monte Carlonprogram are outlined. The code employs an embedded three-level Cartesian mesh accompanied by a cut-cellnalgorithmto incorporate triangulated surface geometry. A simple and efficient adaptivemesh refinement algorithmnthatmaintains a local cell size and time step consistent with the local mean-free path and local mean-collision time isndetailed, along with a cut-cell algorithm that sorts triangulated surface elements into Cartesian cells and uses anMonte Carlo technique to compute the cut volume. Three-dimensional direct simulationMonte Carlo simulations ofnhypersonic flow over a 70 deg blunted cone geometry at various angles of attack are presented. For a 0 deg angle ofnattack, direct simulation Monte Carlo solutions are in excellent agreement with other simulations reported in thenliterature and with experimental results for density field and surface heat flux. New simulation results are presentednfor three-dimensional flows over the probe geometry at 10 and 30 deg angles of attack where direct simulationnMonte Carlo predictions for density field and heat flux are in close agreement with the experiment. The largestndiscrepancy is found in the heat flux along thewindward forebody (for 30 deg angles of attack),where the simulationsnoverpredict the experimental measurements by, at most, 25%.
机译:概述了新开发的三维直接仿真Monte Carlonprogram的数据结构和算法。该代码采用嵌入的三级笛卡尔网格,并带有cut-cellnalgorithm来合并三角表面几何形状。一种简单而有效的自适应网格细化算法,该算法保持局部像元大小和时间步长与局部无均值路径和局部平均碰撞时间一致,此外还有一个割格算法,该算法将三角化的表面元素分类为笛卡尔单元,并使用蒙特卡洛技术计算切割量。提出了在70度钝锥几何结构上各种迎角上的非人为流的三维直接模拟的蒙特卡罗模拟。对于攻角为0度的情况,直接模拟蒙特卡洛解决方案与文献中报道的其他模拟以及密度场和表面热通量的实验结果都非常吻合。在10和30度攻角下的探头几何三维流动提出了新的模拟结果,其中直接模拟密度场和热通量的蒙特卡罗预测与实验吻合良好。在沿前体的热通量中(在迎角为30度时)发现最大的偏差,其中模拟最多预测实验测量值不超过25%。

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