Juice/SWI during the Lunar-Earth-Gravity-Assist (LEGA) – Part 4: Antenna pointing and beam characterisation

Abstract. The Submillimetre Wave Instrument (SWI) onboard the Jupiter Icy Moons Explorer (Juice) spacecraft consists of a 29 cm off-axis paraboloid antenna and two double-sideband heterodyne receivers operating in the frequency ranges of 530–638 and 1066–1286 GHz. This instrument is designed to study Jupiter’s atmosphere and the exospheres of the Galilean moons. We used the Lunar-Earth-Gravity-Assist (LEGA) data from August 2024 to characterise this antenna using several SWI observations pointing towards the Earth. The data analysis of the LEGA observations dedicated to the antenna beam allows us to characterise the antenna beam Full Width at Half Maximum (FWHM), sidelobes, absolute pointing and receiver coalignement. Moreover, an estimate of the calibration efficiency factor has been obtained.

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Publication Details

Journal
Annales Geophysicae
Published
2026-10-30
DOI
https://doi.org/10.5194/angeo-44-1227-2026
Citations
3
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
9.17

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article

Juice/SWI during the Lunar-Earth-Gravity-Assist (LEGA) – Part 4: Antenna pointing and beam characterisation

B. Dąbrowski, Mikko Kotiranta, P. Hartogh, S. Szutowicz et al.
3 citations
Annales Geophysicae
Radio Astronomy Observations and Technology
9.17
article

Juice/SWI during the Lunar-Earth-Gravity-Assist (LEGA) – Part 4: Antenna pointing and beam characterisation

B. Dąbrowski, Mikko Kotiranta, P. Hartogh, S. Szutowicz, R. Moreno, Donal P. Murtagh, F. Herpin, Hideo Sagawa, Thibault Cavalié, L. Rezac, Axel Murk, Tomáš Formánek, E. Lellouch, Yasuko J. Kasai, M. Rengel, C. Jarchow, Samuel Goodyear, Ali Schulz-Ravanbakhsh, Alberto Carrasco Gallardo, Eva Wirström, Michael Olberg
article en
3 citations

Abstract

Abstract. The Submillimetre Wave Instrument (SWI) onboard the Jupiter Icy Moons Explorer (Juice) spacecraft consists of a 29 cm off-axis paraboloid antenna and two double-sideband heterodyne receivers operating in the frequency ranges of 530–638 and 1066–1286 GHz. This instrument is designed to study Jupiter’s atmosphere and the exospheres of the Galilean moons. We used the Lunar-Earth-Gravity-Assist (LEGA) data from August 2024 to characterise this antenna using several SWI observations pointing towards the Earth. The data analysis of the LEGA observations dedicated to the antenna beam allows us to characterise the antenna beam Full Width at Half Maximum (FWHM), sidelobes, absolute pointing and receiver coalignement. Moreover, an estimate of the calibration efficiency factor has been obtained.

Annales GeophysicaeVol. 44(2)
University of Bern (CH), Centrum Badań Kosmicznych (PL), Centre National de la Recherche Scientifique (FR), Université de Bordeaux (FR), Kyoto Sangyo University (JP), Université Paris Cité (FR), Université Paris Sciences et Lettres (FR), Observatoire de Paris (FR), Sorbonne Université (FR), Laboratoire d'Astrophysique de Bordeaux (FR), Max Planck Institute for Solar System Research (DE), Institute of Science Tokyo (JP), LIRA - Laboratoire d'instrumentation et de recherche en astrophysique (FR), Chalmers University of Technology (SE), National Institute of Information and Communications Technology (JP), Polish Academy of Sciences (PL)
European Space Agency, Agence Nationale de la Recherche, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Swedish National Space Agency
Openalex Percentile: Top 2%
Radio Astronomy Observations and Technology
9.17
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