Overview of the Delay Doppler Mapping Instrument (DDMI) for the cyclone global navigation satellite systems mission (CYGNSS)

S. Gleason, C. Ruf
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引用次数: 9

Abstract

The CYGNSS satellite constellation consists of eight satellites equipped with GNSS bi-static radar receivers which map the ocean surface scattered signal power in the vicinity of the specular reflection point using time domain and Doppler frequency filters. The satellites orbit in the same plane at an altitude of 500 km and at a orbit inclination of 35 degrees. CYGNSS will act as a GNSS bi-static scatterometer capable of sensing sea level winds in tropical cyclones, including in high precipitation conditions. An overview of the GNSS remote sensing concept is included in this paper. Subsequently, an overview of the Delay Doppler Mapping Instrument (DDMI) carried by all of the CYGNSS observatories will be presented. The DDMI uses GPS forward scattered signals of opportunity to produce delay Doppler maps (DDMs) of the scattered signal delay and frequency spreading over the surface. This paper will conclude with results from preliminary laboratory testing of the CYGNSS instrument engineering models.
用于气旋全球导航卫星系统任务(CYGNSS)的延迟多普勒测绘仪(DDMI)概述
CYGNSS卫星星座由8颗卫星组成,配备GNSS双基地雷达接收机,利用时域和多普勒频率滤波器绘制镜面反射点附近的海面散射信号功率。两颗卫星在同一平面上运行,轨道倾角为35度,高度为500公里。CYGNSS将作为GNSS双静态散射计,能够在热带气旋中感知海平面风,包括在高降水条件下。本文概述了GNSS遥感的概念。随后,将介绍所有CYGNSS天文台携带的延迟多普勒测绘仪器(DDMI)的概述。DDMI使用GPS前向散射信号的机会产生散射信号的延迟多普勒图(DDMs)的延迟和频率在地面上扩散。本文将以CYGNSS仪器工程模型的初步实验室测试结果作为结论。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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