satellite antenna
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2022 ◽  
Vol 2160 (1) ◽  
pp. 012037
Author(s):  
Yuying Chen ◽  
Jing Li ◽  
Wei Zhang ◽  
Bin He

Abstract Ring truss antenna is an ideal structure for large satellite antenna, which can be equivalent to circular cylindrical shell model. Based on the high-dimensional nonlinear dynamic vibration and bifurcation theory, we focus on the nonlinear dynamic behavior for breathing vibration system of ring truss antenna with internal resonance. The nonlinear transformation and Routh-Hurwitz criterion are used to analyze the stability of equilibrium point after disturbance, and the theoretical analysis is verified by numerical simulation. It provides a reference to ensure the stability and control parameters of satellite antenna in complex space environment.


2021 ◽  
Author(s):  
Stirling MacPherson ◽  
Roger Irakoze ◽  
Eagan Boire ◽  
Darvin Patel ◽  
Cole Hawes ◽  
...  

GPS Solutions ◽  
2021 ◽  
Vol 25 (3) ◽  
Author(s):  
Susanne Beer ◽  
Lambert Wanninger ◽  
Anja Heßelbarth

AbstractGNSS satellite and receiving antennas exhibit group delay variations (GDV), which affect code pseudorange measurements. Like antenna phase center variations, which affect phase measurements, they are frequency-dependent and vary with the direction of the transmitted and received signal. GNSS code observations contain the combined contributions of satellite and receiver antennas. If absolute GDV are available for the receiver antennas, absolute satellite GDV can be determined. In 2019, an extensive set of absolute receiver antenna GDV was published and, thus, it became feasible to estimate absolute satellite antenna GDV based on terrestrial observations. We used the absolute GDV of four selected receiver antenna types and observation data of globally distributed reference stations that employ these antenna types to determine absolute GDV for the GPS, GLONASS, Galileo, BeiDou, and QZSS satellite antennas. Besides BeiDou-2 satellites whose GDV are known to reach up to 1.5 m peak-to-peak, the GPS satellites show the largest GDV at frequencies L1 and L5 with up to 0.3 and 0.4 m peak-to-peak, respectively. They also show the largest satellite-to-satellite variations within a constellation. The GDV of GLONASS-M satellites reach up to 25 cm at frequency G1; Galileo satellites exhibit the largest GDV at frequency E6 with up to 20 cm; BeiDou-3 satellites show the largest GDV of around 15 cm at frequencies B1-2 and B3. Frequencies L2 of GPS IIIA, E1 of Galileo FOC, and B2a/B2b of BeiDou-3 satellites are the least affected. Their variations are below 10 cm.


2021 ◽  
Author(s):  
Lili Zhao ◽  
Pengpeng Yu ◽  
Qicai Dong ◽  
Xianglei Meng ◽  
Xiangyang Huang ◽  
...  
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2021 ◽  
Vol 1885 (5) ◽  
pp. 052001
Author(s):  
Li yu-hua ◽  
Liu Bo Xue ◽  
Zhang Xiao Bo ◽  
Zhao Feng ◽  
Jing Li-Li

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