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Record W4405417590 · doi:10.1007/s11214-024-01110-0

The Radio & Plasma Wave Investigation (RPWI) for the JUpiter ICy moons Explorer (JUICE)

2024· article· en· W4405417590 on OpenAlexaff
Jan‐Erik Wahlund, J. E. S. Bergman, L. Åhlén, W. Puccio, Baptiste Cecconi, Yasumasa Kasaba, Hanna Rothkaehl, Marek Morawski, O. Santolı́k, J. Souček, Jerzy Grygorczuk, Ł. Wiśniewski, Pierre Henri, J. L. Rauch, Olivier Le Duff, Alessandro Retinò, Malik Mansour, Š. Štverák, J. Laifr, D. J. Andrews, M. André, Igor Benko, Martina Berglund, V. Cripps, C. M. Cully, Jan Davidsson, A. P. Dimmock, N. J. T. Edberg, A. I. Eriksson, Johan Fredriksson, R. Gill, Stéphane Gomis, B. Holback, S.-E. Jansson, F. Johansson, E. P. G. Johansson, Y. V. Khotyaintsev, Björn Mårtensson, M. Morooka, Thomas Nilsson, D. Ohlsson, D. Pelikan, Louis Richard, F. Shiwa, E. Vigren, Harvey Wong, X. Bonnin, J. N. Girard, Lucas Grosset, Florence Henry, Laurent Lamy, J. P. Lebreton, P. Zarka, Yuto Katoh, Hajime Kita, Atsushi Kumamoto, Hiroaki Misawa, Fuminori Tsuchiya, M. Galand, Tomasz Barciński, Jakub Baran, Tomasz Kowalski, P. Szewczyk, B. Grison, Jacqueline H. Jansky, Ivana Kolmašová, Radek Lán, Ulrich Taubenschuss, K. Bochra, Michał Borys, Marcin Duda, T. Kuciński, Marek Ossowski, Paolo Palma, M. Tokarz, Fabrice Colin, Patrizio Dazzi, Emmanuel De Leon, T. Hachemi, Aude-Lyse Millet, O. Randrianboarisson, O. Sene, T. Chust, O. Le Contel, P. Canu, Lina Hadid, F. Sahraoui, I. Zouganelis, D. Alison, Brett A. Neilan, Alexis Jeandet, Mathieu Lebassard, Jean‐Denis Techer, Fatima Mehrez, Laurent Varizat, Anirudha V. Sumant, G. Sou, Petr Hellinger, P. Trávnı́ček, L. Bylander, Gabriel Giono, Nickolay Ivchenko, Anita Kullen, Lorenz Roth, A. Vaivads, K. Tanimoto, Hiroyuki Mizuno, Akihiko Sawamura, T. Suzuki, Masatoshi Namiki, Satoshi Fujishima, K. Asai, Tetsuya Shimoyama, Masayuki Fujii, Yuki Sato, Jens Birch, Babak Bakhit, Grzegorz Greczyński, P. Gare, Sven Landström, R. LeLetty, Ewelina Ryszawa, I. Torralba, Jorge Lopez Trescastro, S. Osipenco, Urban Wiklund, A. Roos, Johan Söderström, Olle Björneholm, G. Fischer, Tomas Nyberg, Kiran Kumar Kovi, М. А. Балихин, K. H. Yearby, Mika Holmberg, C. M. Jackman, Corentin Louis, Amine Rhouni, Vincent Leray, N. Geyskens, Christophe Berthod, Bruno J. Lemaire, Aurélien Clémençon, Gaëtan Wattieaux, Nicolás André, Philippe Garnier, V. Génot, P. Louarn, A. Marchaudon, R. Modolo, Claire Baskevitch, L. Hess, Ludivine Leclercq, Joachim Saur, Tomoki Kimura, Hirotsugu Kojima, Satoshi Yagitani, Yoshizumi Miyoshi

Bibliographic record

VenueSpace Science Reviews · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsUniversity of Calgary
FundersBasic Energy SciencesScience and Technology Facilities CouncilOffice of ScienceCentre National de la Recherche ScientifiqueJapan Aerospace Exploration AgencyU.S. Department of EnergyCentre National d’Etudes SpatialesUppsala UniversitetSwedish National Space AgencyScience Foundation Ireland
KeywordsIcy moonPhysicsIonospherePlasmaJupiter (rocket family)JovianGeophysicsSpacecraftRemote sensingAstronomyPlanetGeology

Abstract

fetched live from OpenAlex

Abstract The Radio & Plasma Wave Investigation (RPWI) onboard the ESA JUpiter ICy moons Explorer (JUICE) is described in detail. The RPWI provides an elaborate set of state-of-the-art electromagnetic fields and cold plasma instrumentation, including active sounding with the mutual impedance and Langmuir probe sweep techniques, where several different types of sensors will sample the thermal plasma properties, including electron and ion densities, electron temperature, plasma drift speed, the near DC electric fields, and electric and magnetic signals from various types of phenomena, e.g., radio and plasma waves, electrostatic acceleration structures, induction fields etc. A full wave vector, waveform, polarization, and Poynting flux determination will be achieved. RPWI will enable characterization of the Jovian radio emissions (including goniopolarimetry) up to 45 MHz, has the capability to carry out passive radio sounding of the ionospheric densities of icy moons and employ passive sub-surface radar measurements of the icy crust of these moons. RPWI can also detect micrometeorite impacts, estimate dust charging, monitor the spacecraft potential as well as the integrated EUV flux. The sensors consist of four 10 cm diameter Langmuir probes each mounted on the tip of 3 m long booms, a triaxial search coil magnetometer and a triaxial radio antenna system both mounted on the 10.6 m long MAG boom, each with radiation resistant pre-amplifiers near the sensors. There are three receiver boards, two Digital Processing Units (DPU) and two Low Voltage Power Supply (LVPS) boards in a box within a radiation vault at the centre of the JUICE spacecraft. Together, the integrated RPWI system can carry out an ambitious planetary science investigation in and around the Galilean icy moons and the Jovian space environment. Some of the most important science objectives and instrument capabilities are described here. RPWI focuses, apart from cold plasma studies, on the understanding of how, through electrodynamic and electromagnetic coupling, the momentum and energy transfer occur with the icy Galilean moons, their surfaces and salty conductive sub-surface oceans. The RPWI instrument is planned to be operational during most of the JUICE mission, during the cruise phase, in the Jovian magnetosphere, during the icy moon flybys, and in particular Ganymede orbit, and may deliver data from the near surface during the final crash orbit.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.002
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.871
Threshold uncertainty score0.807

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0020.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.066
GPT teacher head0.296
Teacher spread0.230 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designNot applicable
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations7
Published2024
Admission routes1
Has abstractyes

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