

Author: Gao Fan Xu Tianhe Wang Nazi Jiang Chunhua Du Yujun Nie Wenfeng Xu Guochang
Publisher: MDPI
E-ISSN: 2072-4292|10|1|67-67
ISSN: 2072-4292
Source: Remote Sensing, Vol.10, Iss.1, 2018-01, pp. : 67-67
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Spaceborne GNSS-R (global navigation satellite system reflectometry) is an innovative and powerful bistatic radar remote sensing technique that uses specialized GNSS-R instruments on LEO (low Earth orbit) satellites to receive GNSS L-band signals reflected by the Earth’s surface. Unlike monostatic radar, the illuminated areas are elliptical regions centered on specular reflection points. Evaluation of the spatiotemporal resolution of the reflections is necessary at the GNSS-R mission design stage for various applications. However, not all specular reflection signals can be received because the size and location of the GNSS-R antenna’s available reflecting ground coverage depends on parameters including the on-board receiver antenna gain, the signal frequency and power, the antenna face direction, and the LEO’s altitude. Additionally, the number of available reflections is strongly related to the number of GNSS-R LEO and GNSS satellites. By 2020, the Galileo and BeiDou Navigation Satellite System (BDS) constellations are scheduled to be fully operational at global scale and nearly 120 multi-GNSS satellites, including Global Positioning System (GPS) and Global Navigation Satellite System (GLONASS) satellites, will be available for use as illuminators. In this paper, to evaluate the future capacity for repetitive GNSS-R observations, we propose a GNSS satellite selection method and simulate the orbit of eight-satellite LEO and partial multi-GNSS constellations. We then analyze the spatiotemporal distribution characteristics of the reflections in two cases: (1) When only GPS satellites are available; (2) when multi-GNSS satellites are available separately. Simulation and analysis results show that the multi-GNSS-R system has major advantages in terms of available satellite numbers and revisit times over the GPS-R system. Additionally, the spatial density of the specular reflections on the Earth’s surface is related to the LEO inclination and constellation construction.
Related content


An Optimal Tropospheric Tomography Method Based on the Multi-GNSS Observations
By Zhao Qingzhi Yao Yibin Cao Xinyun Zhou Feng Xia Pengfei
Remote Sensing, Vol. 10, Iss. 2, 2018-02 ,pp. :


Investigation on Reference Frames and Time Systems in Multi-GNSS
By Nicolini Luca Caporali Alessandro
Remote Sensing, Vol. 10, Iss. 1, 2018-01 ,pp. :




Weighting of Multi-GNSS Observations in Real-Time Precise Point Positioning
By Kazmierski Kamil Hadas Tomasz Sośnica Krzysztof
Remote Sensing, Vol. 10, Iss. 1, 2018-01 ,pp. :