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超重星舰一子级气动返回阶段底部载荷研究

林晓辉 高武焕 秦曈 陈立为 楚宜慧 薛飞 顾远富 许常悦

林晓辉, 高武焕, 秦曈, 等. 超重星舰一子级气动返回阶段底部载荷研究[J]. 航空动力学报, 2026, 41(5):20250221 doi: 10.13224/j.cnki.jasp.20250221
引用本文: 林晓辉, 高武焕, 秦曈, 等. 超重星舰一子级气动返回阶段底部载荷研究[J]. 航空动力学报, 2026, 41(5):20250221 doi: 10.13224/j.cnki.jasp.20250221
LIN Xiaohui, GAO Wuhuan, QIN Tong, et al. Investigation of base load characteristics during aerodynamic reentry phase of super heavy starship[J]. Journal of Aerospace Power, 2026, 41(5):20250221 doi: 10.13224/j.cnki.jasp.20250221
Citation: LIN Xiaohui, GAO Wuhuan, QIN Tong, et al. Investigation of base load characteristics during aerodynamic reentry phase of super heavy starship[J]. Journal of Aerospace Power, 2026, 41(5):20250221 doi: 10.13224/j.cnki.jasp.20250221

超重星舰一子级气动返回阶段底部载荷研究

doi: 10.13224/j.cnki.jasp.20250221
基金项目: 国家自然科学基金(12172172); 江苏高校优势学科建设工程资助项目;战略火箭创新基金(ZH2024003)
详细信息
    作者简介:

    林晓辉(1996-),男,博士生,主要研究方向为火箭湍流数值模拟及流动控制。E-mail:xh-lin@nuaa.edu.cn

    通讯作者:

    许常悦(1981-),男,副教授,博士,主要研究方向为可压缩湍流数值模拟。E-mail:cyxu@nuaa.edu.cn

  • 中图分类号: V421.4

Investigation of base load characteristics during aerodynamic reentry phase of super heavy starship

  • 摘要:

    垂直返回可重复使用火箭在返回气动减速阶段由于火箭底部为迎风面,对底部发动机喷管的力、热特性产生显著影响。采用计算流体力学方法对超重星舰一子级火箭底部的流动特性进行数值模拟,获得了火箭在典型气动减速段工况马赫数为3.5、攻角为0°~15°范围的流场结构及底部喷管的载荷分布。结果表明:火箭返回时底部形成了随攻角变化的弓形激波,在背风侧形成了大尺度的流动分离;外圈、中圈和内圈喷管所受侧向载荷之比为335∶19∶1,呈指数级下降;随着攻角增加,喷管侧向载荷从背风侧向迎风侧逐渐减小。气动热对火箭底部以及外圈喷管的影响显著。研究结果可为垂直返回火箭底部发动机的布局及气动减速阶段的姿态控制方案提供理论支撑。

     

  • 图 1  星舰第5次试验助推器返回时速度剖面

    Figure 1.  Velocity profile of the starship booster during the fifth test flight

    图 2  计算域示意图

    Figure 2.  Schematic of the computational domain

    图 3  底部喷管分布

    Figure 3.  Distribution of the nozzle at the bottom

    图 4  气动力验证结果

    Figure 4.  Results of aerodynamic verification

    图 5  气动热验证结果

    Figure 5.  Results of the aerodynamic thermal verification

    图 6  不同网格计算结果

    Figure 6.  Calculation results of different grids

    图 7  对称截面(Y-Z截面)的马赫数分布

    Figure 7.  Mach number distribution on the symmetric (Y-Z) plane

    图 8  Z = −3.5 截面处的Lamb矢量散度云图

    Figure 8.  Contours of Lamb vector divergence on thez = −3.5 plane

    图 9  根据${\lambda _2}$准则绘制的涡结构

    Figure 9.  Vortex structures described based on ${\lambda _2}$ criterion

    图 10  子级火箭底部温度分布

    Figure 10.  Temperature distribution on the base of the Starship lower stage

    图 11  喷管侧向载荷$ {\tilde f_{{\text{side}}}} $分布

    Figure 11.  Side loads $ {\tilde f_{{\text{side}}}} $ distribution on the nozzle

    图 12  喷管轴向载荷$ {\tilde f_{{\text{axial}}}} $分布

    Figure 12.  Axial loads $ {\tilde f_{{\text{axial}}}} $ distribution on the nozzle

    图 13  不同攻角下喷管壁面压力分布

    Figure 13.  Pressure distribution on the nozzle wall at different angles of attack

    图 14  喷管压力采样位置

    Figure 14.  Nozzle wall pressure sampling locations

    图 15  底面无量纲压力分布

    Figure 15.  Non-dimensional pressure distribution on the bottom

    图 16  底面无量纲温度分布

    Figure 16.  Non-dimensional temperature distribution on the bottom

    图 17  底面无量纲压力分布曲线

    Figure 17.  Non-dimensional pressure distribution curve on the bottom

    图 18  底面无量纲温度分布曲线

    Figure 18.  Non-dimensional temperature distribution curve on the bottom

    表  1  几何参数表

    Table  1.   Geometry parameters m

    几何参数 数值
    火箭直径D 9.00
    内圈半径${r_3}$ 0.78
    中圈半径${r_2}$ 2.36
    外圈半径${r_1}$ 4.03
    喷管高度h 0.69
    喷管出口半径r 0.58
    喷管突出距离ΔL 0.30
    下载: 导出CSV
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  • 收稿日期:  2025-05-08
  • 网络出版日期:  2025-10-22

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