Juno Radio Open Loop Measurement Experiment based on China’s Deep Space Stations

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  • 1. Beijing Aerospace Control Center,Beijing 100094,China;
    2. National Astronomical Observatories, CAS,Beijing 100012,China;
    3. Xinjiang Astronomical Observatory,CAS,Urumqi 830011,China;
    4. Xi’an Satellite Control Center,Xi’an 710043,China;
    5. Shanghai Astronomical Observatory,CAS,Shanghai 200030,China

Received date: 20 Oct 2017

Revised date: 21 Mar 2018

Abstract

The construction of China’s deep space network supports China’s deep space missions,such as explorations of Lunar,Mars,Small planets,Jupiter,and etc. To validate China’s deep space network performance and obtain the radio measurement raw data,dozens of radio open loop measurement experiments of Juno which is one of Jupiter’s probe on orbit were accomplished. These open loop measurement experiments are the first time conducted by the China’s deep space stations tracking a in-orbit probe in Earth-Jupiter distance. VLBI terminate sampling and recording facilities were utilized to record Juno’s raw carrier signal,which was processed to extract Doppler frequency between Juno and the deep space station. In this paper,the combining method of Fast Fourier transform,Chirp Z transform and signal local reconstruction was utilized to obtain Juno’s Doppler frequency. The results show that Juno’s open loop Doppler frequency is at the level of 10 μHz,which effectively validated the method of deep space open loop measurement and provide valuable reference for China’s future deep space missions.

Cite this article

CHEN Lue, PING Jinsong, LI Wenxiao, HAN Songtao, LIU Qing, CHEN Yongqiang, ZHANG Jianhui, JIAN Nianchuan . Juno Radio Open Loop Measurement Experiment based on China’s Deep Space Stations[J]. Journal of Deep Space Exploration, 2018 , 5(4) : 382 -386 . DOI: 10.15982/j.issn.2095-7777.2018.04.009

References

[1] MATOUSEK S. The Juno New Frontiers mission[J]. Acta Astronautica,2007,61:932-939
[2] SERRAA D,DIMAREB L,TOMMEIA G,et al. Gravimetry,rotation and angular momentum of Jupiter from the Juno Radio Science experiment[J]. Planetary and Space Science,2016,134(1):100-111
[3] WILSON H F. Diffusivity of heavy elements in Jupiter and Saturn[J]. Icarus,2015,250:400-404
[4] MUKAI R,HANSEN D,MITTSKUS A,et al. Juno telecommunications[R]. California:Jet Propulsion Laboratory,California Institute of Technology,2012.
[5] 平劲松,尚堃,钱志瀚,等. 萤火一号火星轨道器开环追踪技术[J]. 航天器工程,2009,18(5):6-11
PING J S,SHANG K,QIAN Z H,et al. Open loop tracking for Yinghuo-1 Martian orbiter[J]. Spacecraft Engineering,2009,18(5):6-11
[6] 陈略,唐歌实,孟桥,等. 一种卫星信号频率精确估计方法研究及应用[J]. 遥测遥控,2010,31(6):26-30
CHEN L,TANG G S,MENG Q,et al. Research and application of satellite signal frequency accurate estimation method[J]. Journal of Telemetry,Tracking and Command,2010,31(6):26-30
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