探测朱诺号的“心跳”:朱诺号任务关键事件期间的通信支持

D. Buccino, M. Soriano, K. Oudrhiri, S. Finley, D. Kahan, O. Yang, A. Jongeling
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引用次数: 2

摘要

自发射以来,无线电科学一直是朱诺号木星任务的关键组成部分。无线电科学研究的主要目标是通过航天器与美国宇航局深空网络(DSN)的地面观测天线之间的无线电链路的多普勒频移来估计木星的引力场。除了对引力场的估计,无线电科学还为朱诺号任务提供了关键的工程支持。利用高灵敏度的开环接收器和实时信号处理,无线电科学能够探测到朱诺号航天器的“心跳”,并确定航天器的当前状态。朱诺号航天器利用两个频率与地球通信:电信系统x波段链路和无线电科学ka波段链路。无线电科学为2011年的航天器发射、航天器主发动机点火(包括2012年的深空机动和2016年的木星轨道插入)、2013年的地球重力辅助飞越以及航天器在木星最接近时的微弱信号水平离地点提供了通信监测支持。通过实时测量x波段下行信号的信噪比、接收的载波频率和副载波频率,无线电科学能够在链路余量不足以支持遥测的情况下确定航天器的状态。非标称航天器状态将改变信号噪声水平、子载波频率和载波频率的自旋调制,这些在深空网络的开环接收器中可检测到。通过增加多频移键控(MFSK)“音调”编码,可以在航天器上改变副载波频率,以确定飞行团队选择的事件。在朱诺号的主发动机点火期间,包括木星轨道插入(JOI),都使用了音调。音调由DSN开环接收机下游的进入、下降和着陆(EDL)数据分析(EDA)系统近乎实时地解码。硬件、软件和操作计划的稳健实施确保了成功的数据收集和向朱诺号任务报告航天器状态的实时状态。在木星恶劣的环境中,以这种方式与朱诺号交流的经验教训被记录下来,并在即将到来的木星任务中进行讨论。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Detecting Juno's ‘Heartbeat’: Communications Support during Critical Events of the Juno Mission
Since launch, radio science has been a key component of the Juno mission to Jupiter. The prime objective of the radio science investigation is to estimate the gravitational field of Jupiter from the Doppler shift on the radio link between the spacecraft and the Earth-based observing antennas of NASA's Deep Space Network (DSN). In addition to estimation of the gravitational field, radio science has provided critical engineering support to the Juno mission. Utilizing high-sensitivity open-loop receivers and real-time signal processing, radio science is able to detect the ‘heartbeat’ of the Juno spacecraft and determine the current state of the spacecraft. The Juno spacecraft utilizes two frequencies for communication with Earth: the telecommunications system X-band link and the radio science Ka-band link. Radio science has provided communications monitoring support for the spacecraft launch in 2011, spacecraft main engine firings (including Deep Space Maneuvers in 2012 and Jupiter Orbit Insertion in 2016), the Earth gravity assist flyby in 2013, and times when the spacecraft was off-Earth point during Jupiter closest approach with a weak signal level. By measuring the signal-to-noise ratio, received carrier frequency, and subcarrier frequency of the X-band downlink signal in real-time, radio science is able to determine the state of the spacecraft in scenarios where the link margin is not sufficient to support telemetry. An off-nominal spacecraft state will change the signal-to-noise level, subcarrier frequency, and spin modulation of the carrier frequency which are detectable in the open-loop receiver of the DSN. With the addition of multiple frequency shift keying (MFSK) ‘tones’ encoding, the subcarrier frequency can be changed onboard the spacecraft for determination of selected events by the flight team. Tones were utilized during main engine firings on Juno, including Jupiter Orbit Insertion (JOI). Tones are decoded in near real-time by the Entry, Descent, and Landing (EDL) Data Analysis (EDA) system downstream of the DSN open-loop receivers. Robust implementation of hardware, software, and operations planning has ensured successful data collection and real-time status reporting of spacecraft state to the Juno mission. Lessons learned from communicating with Juno in this way while in the harsh environment of Jupiter are documented and discussed in the context of upcoming missions to Jupiter.
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