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Jupiter Science Enabled by ESA’s Jupiter Icy Moons Explorer
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SYSNO ASEP 0576125 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Jupiter Science Enabled by ESA’s Jupiter Icy Moons Explorer Tvůrce(i) Fletcher, L. N. (GB)
Cavalié, T. (FR)
Grassi, D. (IT)
Hueso, R. (ES)
Lara, L. M. (ES)
Kaspi, Y. (IL)
Galanti, E. (IL)
Greathouse, T. K. (GB)
Molyneux, P. M. (GB)
Galand, M. (GB)
Vallat, C. (ES)
Witasse, O. (NL)
Lorente, R. (ES)
Hartogh, P. (DE)
Poulet, F. (FR)
Langevin, Y. (FR)
Palumbo, P. (IT)
Gladstone, G.R. (US)
Retherford, K. D. (US)
Dougherty, M. K. (GB)
Wahlund, J.-E. (SE)
Barabash, S. (SE)
Iess, L. (IT)
Bruzzone, L. (IT)
Hussmann, H. (DE)
Gurvits, L. I. (NL)
Santolík, Ondřej (UFA-U) RID, ORCID
Kolmašová, Ivana (UFA-U) RID, ORCID
Fischer, G. (AT)
Müller-Wodarg, I. (GB)
Piccioni, G. (IT)
Fouchet, T. (FR)
Gérard, J. C. (BE)
Sánchez-Lavega, A. (ES)
Irwin, P. G.J. (GB)
Grodent, D. (BE)
Altieri, F. (IT)
Mura, A. (IT)
Drossart, P. (FR)
Kammer, J. (US)
Giles, R. (US)
Cazaux, S. (NL)
Jones, G. (GB)
Smirnova, M. (IL)
Lellouch, E. (FR)
Medvedev, A. S. (DE)
Moreno, R. (FR)
Rezac, L. (DE)
Coustenis, A. (FR)
Costa, M. (ES)Celkový počet autorů 50 Číslo článku 53 Zdroj.dok. Space Science Reviews. - : Springer - ISSN 0038-6308
Roč. 219, č. 7 (2023)Poč.str. 75 s. Jazyk dok. eng - angličtina Země vyd. DE - Německo Klíč. slova Atmospheres ; Auroras ; Chemistry ; Dynamics ; juice ; Jupiter Vědní obor RIV BL - Fyzika plazmatu a výboje v plynech Obor OECD Fluids and plasma physics (including surface physics) Způsob publikování Open access Institucionální podpora UFA-U - RVO:68378289 UT WOS 001072292500001 EID SCOPUS 85171878271 DOI https://doi.org/10.1007/s11214-023-00996-6 Anotace ESA’s Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital tour tailored to maximise observing opportunities. We review the Jupiter science enabled by the JUICE mission, building on the legacy of discoveries from the Galileo, Cassini, and Juno missions, alongside ground- and space-based observatories. We focus on remote sensing of the climate, meteorology, and chemistry of the atmosphere and auroras from the cloud-forming weather layer, through the upper troposphere, into the stratosphere and ionosphere. The Jupiter orbital tour provides a wealth of opportunities for atmospheric and auroral science: global perspectives with its near-equatorial and inclined phases, sampling all phase angles from dayside to nightside, and investigating phenomena evolving on timescales from minutes to months. The remote sensing payload spans far-UV spectroscopy (50-210 nm), visible imaging (340-1080 nm), visible/near-infrared spectroscopy (0.49-5.56 μm), and sub-millimetre sounding (near 530-625 GHz and 1067-1275 GHz). This is coupled to radio, stellar, and solar occultation opportunities to explore the atmosphere at high vertical resolution: and radio and plasma wave measurements of electric discharges in the Jovian atmosphere and auroras. Cross-disciplinary scientific investigations enable JUICE to explore coupling processes in giant planet atmospheres, to show how the atmosphere is connected to (i) the deep circulation and composition of the hydrogen-dominated interior: and (ii) to the currents and charged particle environments of the external magnetosphere. JUICE will provide a comprehensive characterisation of the atmosphere and auroras of this archetypal giant planet. Pracoviště Ústav fyziky atmosféry Kontakt Kateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019 Rok sběru 2024 Elektronická adresa https://link.springer.com/article/10.1007/s11214-023-00996-6
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