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基于DSMC方法的再入飞行器微烧蚀研究

甘驰,陈松,张俊

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甘驰, 陈松, 张俊. 基于DSMC方法的再入飞行器微烧蚀研究. 力学学报, 2023, 55(9): 1847-1857 doi: 10.6052/0459-1879-23-112
引用本文: 甘驰, 陈松, 张俊. 基于DSMC方法的再入飞行器微烧蚀研究. 力学学报, 2023, 55(9): 1847-1857doi:10.6052/0459-1879-23-112
Gan Chi, Chen Song, Zhang Jun. DSMC study of micro-ablation for reentry vehicles. Chinese Journal of Theoretical and Applied Mechanics, 2023, 55(9): 1847-1857 doi: 10.6052/0459-1879-23-112
Citation: Gan Chi, Chen Song, Zhang Jun. DSMC study of micro-ablation for reentry vehicles.Chinese Journal of Theoretical and Applied Mechanics, 2023, 55(9): 1847-1857doi:10.6052/0459-1879-23-112

基于DSMC方法的再入飞行器微烧蚀研究

doi:10.6052/0459-1879-23-112
基金项目:国家自然科学基金资助项目(12272028)
详细信息
    通讯作者:

    陈松, 副教授, 主要研究方向为稀薄气体动力学与高超声速烧蚀. E-mail:chensong@buaa.edu.cn

  • 中图分类号:V411.8

DSMC STUDY OF MICRO-ABLATION FOR REENTRY VEHICLES

  • 摘要:高超声速再入飞行器面临着严峻的气动热环境, 准确预测微烧蚀过程对热防护系统的设计至关重要. 由于烧蚀会改变气动外形, 进而影响周围的气动热环境以及烧蚀过程本身, 因此需要将烧蚀过程与流场变化进行耦合计算. 文章采用基于直接模拟蒙特卡洛(DSMC)方法的开源程序SPARTA, 对高超声速条件下的再入飞行器表面微烧蚀问题展开研究. 为构建并测试通用的耦合算法, 通过典型的一维烧蚀模型改进了SPARTA的动能烧蚀模型并采用烧蚀表面热平衡模型计算烧蚀速率, 结合Marching Square算法的特点修改了网格节点的计算方法. 针对柱体、球锥以及带有微小粗糙元的斜楔体等典型外形, 文中计算了二维条件下不同气动外形的烧蚀过程并进行了详细分析. 其中球锥截面烧蚀预测结果中沿驻点线的烧蚀面呈现出较快的衰退速率, 并且与文献中驻点附近的结果吻合情况较好. 斜楔体的烧蚀结果表明, 微小粗糙元的附近存在着非常稀薄的流场区域, 并且其与头部驻点区域会率先发生烧蚀, 反映了再入飞行器表面的微烧蚀特征. 烧蚀结果对高超声速下微烧蚀机理的研究以及热防护系统的设计具有参考意义.

  • 图 1SPARTA基本工作流程图

    Figure 1.The basic flowchart of SPARTA

    图 2Marching Square算法的填充规则

    Figure 2.Look up table of Marching Square algorithm

    图 3SPARTA烧蚀外形划分示意图

    Figure 3.The schematic of how SPARTA generates ablation geometry

    图 4SPARTA烧蚀循环示意图

    Figure 4.Flowchart of ablation cycle in SPARTA

    图 5SPARTA模拟烧蚀过程示意图

    Figure 5.Simulated ablation process of SPARTA

    图 6二维方柱烧蚀过程

    Figure 6.The ablation process of the rectangular cylinder

    图 7二维方柱绕流速度场云图

    Figure 7.The velocity contour of the rectangular cylinder

    图 8二维圆柱烧蚀过程

    Figure 8.The ablation of the two-dimensional cylinder

    图 9二维圆柱绕流温度场云图

    Figure 9.The temperature contour of the two-dimensional cylinder

    图 10球锥截面气动外形

    Figure 10.Aerodynamics geometry of the blunt cone section

    图 11球锥截面烧蚀温度场云图

    Figure 11.The temperature contour of the ablated blunt cone section

    图 12SPARTA预测烧蚀外形与文献[21]结果对比

    Figure 12.The surface recession predicted by SPARTA and the comparison with the result in Ref. [21]

    图 13斜楔体截面外形示意图

    Figure 13.Geometry of the wedge with an obstacle

    图 14带有局部粗糙元的斜楔体烧蚀过程

    Figure 14.The ablation process of the obstacle on the wedge

    图 16带有局部粗糙元的斜楔体克努森数云图

    Figure 16.The Knudsen number contour of the wedge with an obstacle

    图 15带有局部粗糙元的斜楔体温度场云图

    Figure 15.The temperature contour of the wedge with an obstacle

    表 1SPARTA计算参数

    Table 1.Simulation parameters in SPARTA

    Parameter Value Description
    ${\rho _\infty }$ 1.433 × 1020 number density/m−3
    $T_\infty$ 187 particle temperature/K
    $v_\infty$ 6813 stream velocity/(m·s−1)
    ${\rm{d}}x,{\rm{d}}y$ 0.0025 grid size/m
    ${\rm{d}}t$ 4 × 10−7 time step length/s
    ${T_w}$ 1000 wall temperature/K
    下载: 导出CSV

    表 2来流条件以及SPARTA设置

    Table 2.Free stream conditions and SPARTA parameters of the simulated blunt cone

    Parameter Value Description
    $\rho_\infty$ 1.7 × 1021 number density/m−3
    $h$ 70 height/km
    $T_\infty$ 219.58 particle temperature/K
    $v_\infty$ 5800 stream velocity/(m·s−1)
    ${T_{{\rm{wall}}} }$ 4000 temperature of the wall/K
    ${\rm{d}}x,{\rm{d}}y$ 0.0005 grid size/m
    ${\rm{d}}t$ 4 × 10−7 time step length/s
    下载: 导出CSV

    表 3来流条件以及SPARTA设置

    Table 3.Free stream conditions and SPARTA parameters of the simulated wedge

    Parameter Value Description
    $h$ 42.5 height/km
    $T_\infty$ 258.1 particle temperature/K
    $v_\infty$ 2732.6 stream velocity/(m·s−1)
    ${T_{{\rm{wall}}} }$ 360 temperature of the wall/K
    ${\rm{d}}x,{\rm{d}}y$ 0.0002 grid size/m
    $\rho _\infty$ 5.8 × 1022 number density/m−3
    ${\rm{d}}t$ 1 × 10−8 time step length/s
    下载: 导出CSV
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出版历程
  • 收稿日期:2023-03-29
  • 录用日期:2023-08-12
  • 网络出版日期:2023-08-13
  • 刊出日期:2023-09-13

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