Ultra-low-frequency radio astronomy observations from a Seleno-centric orbit

This paper introduces the first results of observations with the Ultra-Long-Wavelength (ULW) —- Low Frequency Interferometer and Spectrometer (LFIS) on board the selenocentric satellite Longjiang-2. We present a brief description of the satellite and focus on the LFIS payload. The in-orbit commissio...

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Veröffentlicht in:Experimental astronomy 2023-01, Vol.56 (1), p.333-353
Hauptverfasser: Jingye, Yan, Wu, Ji, Gurvits, Leonid I, Wu, Lin, Deng, Li, Zhao, Fei, Zhou, Li, Lan Ailan, Fan Wenjie, Yi, Min, Yang, Yang, Yang, Zhen, Wei Mingchuan, Guo Jinsheng, Qiu, Shi, Wu, Fan, Hu Chaoran, Chen, Xuelei, Rothkaehl Hanna, Morawski Marek
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container_end_page 353
container_issue 1
container_start_page 333
container_title Experimental astronomy
container_volume 56
creator Jingye, Yan
Wu, Ji
Gurvits, Leonid I
Wu, Lin
Deng, Li
Zhao, Fei
Zhou, Li
Lan Ailan
Fan Wenjie
Yi, Min
Yang, Yang
Yang, Zhen
Wei Mingchuan
Guo Jinsheng
Qiu, Shi
Wu, Fan
Hu Chaoran
Chen, Xuelei
Rothkaehl Hanna
Morawski Marek
description This paper introduces the first results of observations with the Ultra-Long-Wavelength (ULW) —- Low Frequency Interferometer and Spectrometer (LFIS) on board the selenocentric satellite Longjiang-2. We present a brief description of the satellite and focus on the LFIS payload. The in-orbit commissioning confirmed a reliable operational status of the instrumentation. We also present results of a transition observation, which offers unique measurements on several novel aspects. We estimate the RFI suppression required for such a radio astronomy instrumentation at the Moon-distances from Earth as order of − 80 dB. We analyse a method of separating Earth- and satellite-originated radio frequency interference (RFI). It is found that the RFI level at frequencies lower than a few MHz is smaller than the receiver noise floor.
doi_str_mv 10.1007/s10686-022-09887-0
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subjects Instruments
LF radio
Radio astronomy
Radio frequency interference
title Ultra-low-frequency radio astronomy observations from a Seleno-centric orbit
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