一种双星分布式干涉SAR流场测量的基线设计方法

范黄江 张庆君 刘磊 王志斌 王涛

范黄江, 张庆君, 刘磊, 等. 一种双星分布式干涉SAR流场测量的基线设计方法[J]. 雷达学报(中英文), 待出版. doi: 10.12000/JR26065
引用本文: 范黄江, 张庆君, 刘磊, 等. 一种双星分布式干涉SAR流场测量的基线设计方法[J]. 雷达学报(中英文), 待出版. doi: 10.12000/JR26065
FAN Huangjiang, ZHANG Qingjun, LIU Lei, et al. A baseline design method for interferometric SAR ocean current measurements using a dual-satellite distributed system[J]. Journal of Radars, in press. doi: 10.12000/JR26065
Citation: FAN Huangjiang, ZHANG Qingjun, LIU Lei, et al. A baseline design method for interferometric SAR ocean current measurements using a dual-satellite distributed system[J]. Journal of Radars, in press. doi: 10.12000/JR26065

一种双星分布式干涉SAR流场测量的基线设计方法

DOI: 10.12000/JR26065 CSTR: 32380.14.JR26065
基金项目: 国家自然科学基金(62031005),国家民用航天计划(D040305,D030103)
详细信息
    作者简介:

    范黄江,博士生,主要研究方向为星载合成孔径雷达干涉测量、星载SAR系统设计等

    张庆君,研究员,主要研究方向为卫星微波遥感

    刘 磊,研究员,主要研究方向为合成孔径雷达海洋遥感与系统设计

    王志斌,高级工程师,主要研究方向为星载微波遥感系统设计和信号处理

    王 涛,高级工程师,主要研究方向为星载微波遥感系统设计与控制

    通讯作者:

    张庆君 ztzhangqj@163.com

    责任主编:王岩 Corresponding Editor: WANG Yan

  • 中图分类号: TN957

A Baseline Design Method for Interferometric SAR Ocean Current Measurements Using a Dual-satellite Distributed System

Funds: The National Natural Science Foundation of China (62031005), Civilian Space Programme of China (No: D040305), Civilian Space Programme of China (D030103,D030103)
More Information
  • 摘要: 传统星载SAR单基线顺轨干涉体制因基线固定难以满足复杂海况下海面流场测量需求。针对分布式SAR卫星系统多基线协同测流基线设计的问题,该文在干涉相干性与测流敏感性双重约束下,提出一种面向海流测量的多基线优化设计方法,并推导了多基线加权最小二乘融合反演海面流场的理论精度上界。结果表明,该方法可显著降低径向流速误差;当基线数量增加到一定程度后,精度逼近理论上限。不同海况下,融合误差均满足0.1 m/s的测速精度要求,且X频段和C频段需求的短基线较Ku频段更长。该方法可以有效支撑分布式干涉SAR海流测量卫星系统设计。

     

  • 图  1  一发M 收星座在轨测流示意图

    Figure  1.  Schematic diagram of on-orbit current measurement of the M receiving constellation

    图  2  混合基线斜视卫星几何示意图

    Figure  2.  Schematic diagram of the geometry of a hybrid baseline strabismus satellite

    图  3  不同多视数,流场测量误差随相干系数变化

    Figure  3.  OSC measurement error variation with coherence coefficient under different multi-look numbers

    图  4  一个轨道周期交轨钟摆双星相对位置和基线示意图

    Figure  4.  Schematic diagram of relative position and baseline of pendulum

    图  5  一种典型分布式SAR卫星系统几何构型示意图

    Figure  5.  Schematic illustration of a representative geometric configuration for a distributed SAR system

    图  6  单基线流速测量RMSE随有效基线长度变化示意图

    Figure  6.  Single-baseline velocity measurement RMSE variation with effective baseline length

    图  8  不同海况下多基线加权融合精度随基线数量变化曲线示意图

    Figure  8.  Schematic of the variation curve of multi-baseline weighted fusion accuracy with baseline number under different sea states

    图  7  多基线加权融合精度随基线数量的收敛特性示意图

    Figure  7.  Convergence characteristics of multi-baseline weighted fusion accuracy with the number of baselines

    表  1  交轨钟摆双星编队轨道六根数

    Table  1.   The orbital elements of the pendulum

    卫星半长轴(km)离心率轨道倾角(°)近地点辐角(°)升交点赤经(°)平近点角(°)
    主星7133.1370.000197.4000
    辅星7133.1370.000197.400.00240.0031
    下载: 导出CSV

    表  2  系统仿真参数

    Table  2.   System simulation parameters

    参数 数值
    波长$ \lambda $ 0.022 m
    卫星飞行速度$ {V}_{\text{s}} $ 7400 m/s
    斜视角$ \psi $ 45°
    入射角$ {\theta }_{{i}} $ 30°
    轨道高度$ {H} $ 755 km
    风速$ {U}_{10} $ 3~12 m/s
    径向流速$ {v}_{{\mathrm{r}}} $ 0.05~2.0 m/s
    海面散射系数$ {\sigma }^{0} $ −12.5~−6.2 dB
    噪声等效后向散射系数NESZ −20 dB
    等效多视数$ {N}_{\text{L}} $ 1600
    处理去相干$ {\gamma }_{\text{proc}} $ 0.98
    垂直基线去相干$ {\gamma }_{\text{B}} $ 0.97
    下载: 导出CSV

    表  3  6条基线时间去相干系数汇总表

    Table  3.   Summary of time decorrelation coefficients for six rear-vew baselines

    基线 天线对 物理基线长度 有效顺轨基线长度 时间基线(ms) $ {\gamma }_{\text{temp}} $ 适用场景
    $ {\text{B}}_{1} $ A1-A2 3.5 m 159 $ \lambda $ 0.473 0.992 全海况,高相干
    $ {\text{B}}_{2} $ A2-B1 338 m 1727 $ \lambda $ 5.135 0.377 中-低海况
    $ {\text{B}}_{3} $ B1-B2 3.5 m 159 $ \lambda $ 0.473 0.992 全海况,高相干
    $ {\text{B}}_{4} $ A1-B1 341.5 m 1886 $ \lambda $ 5.608 0.313 中-低海况
    $ {\text{B}}_{5} $ A2-B2 341.5 m 1886 $ \lambda $ 5.608 0.313 中-低海况
    $ {\text{B}}_{6} $ A1-B2 345 m 2045 $ \lambda $ 6.081 0.255 中-低海况,高测流敏感性
    下载: 导出CSV

    表  4  各干涉通道总相干性对比表

    Table  4.   Verification of total coherence for each interferometric channel

    通道 海况$ {U}_{10} $ $ {\gamma }_{\text{SNR}} $ $ {\gamma }_{\text{temp}} $ $ {\gamma }_{\text{total}} $ 是否满足 $ \geq 0.3 $
    短基线(B1) 3 m/s 0.85 1.00 0.81
    7 m/s 0.93 0.99 0.88
    12 m/s 0.96 0.98 0.89
    长基线(B6) 3 m/s 0.85 0.78 0.63
    7 m/s 0.93 0.25 0.23 ×
    12 m/s 0.96 0.02 0.02 ×
    下载: 导出CSV

    表  5  各通道干涉相位模糊约束对比表

    Table  5.   Verification of interferometric phase ambiguity constraints for each channel

    通道 $ {\phi }_{\text{max}} $(rad) $ {\phi }_{\text{max}} \lt \text{π} $ 备注
    短(B1) 0.27 高相干,无模糊
    中(B2) 2.93 接近$ \text{π} $,利用B1解缠
    长(B6) 3.47 × 超出$ \text{π} $,利用B1/B2逐级解缠
    下载: 导出CSV

    表  6  各通道径向流速测量精度对比表

    Table  6.   Verification of phase ambiguity constraints for each channel

    通道$ {\gamma }_{\text{total}} $$ {\sigma }_{\phi } $(rad)$ {\sigma }_{{{v}_{r}}} $(m/s)备注
    短基线(B1)0.880.0130.096高相干,低测流敏感性
    长基线(B6)0.230.1020.059低相干,高测流敏感性
    融合(等效)0.027六基线加权融合后精度
    下载: 导出CSV
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  • 收稿日期:  2026-03-25
  • 修回日期:  2026-06-15

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