BibTex format
@article{Fletcher:2023:10.1007/s11214-023-00996-6,
author = {Fletcher, LN and Cavalié, T and Grassi, D and Hueso, R and Lara, LM and Kaspi, Y and Galanti, E and Greathouse, TK and Molyneux, PM and Galand, M and Vallat, C and Witasse, O and Lorente, R and Hartogh, P and Poulet, F and Langevin, Y and Palumbo, P and Gladstone, GR and Retherford, KD and Dougherty, MK and Wahlund, J-E and Barabash, S and Iess, L and Bruzzone, L and Hussmann, H and Gurvits, LI and Santolik, O and Kolmasova, I and Fischer, G and Müller-Wodarg, I and Piccioni, G and Fouchet, T and Gérard, J-C and Sánchez-Lavega, A and Irwin, PGJ and Grodent, D and Altieri, F and Mura, A and Drossart, P and Kammer, J and Giles, R and Cazaux, S and Jones, G and Smirnova, M and Lellouch, E and Medvedev, AS and Moreno, R and Rezac, L and Coustenis, A and Costa, M},
doi = {10.1007/s11214-023-00996-6},
journal = {Space Science Reviews},
title = {Jupiter science Enabled by ESA's Jupiter Icy Moons Explorer},
url = {http://dx.doi.org/10.1007/s11214-023-00996-6},
volume = {219},
year = {2023}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - 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.
AU - Fletcher,LN
AU - Cavalié,T
AU - Grassi,D
AU - Hueso,R
AU - Lara,LM
AU - Kaspi,Y
AU - Galanti,E
AU - Greathouse,TK
AU - Molyneux,PM
AU - Galand,M
AU - Vallat,C
AU - Witasse,O
AU - Lorente,R
AU - Hartogh,P
AU - Poulet,F
AU - Langevin,Y
AU - Palumbo,P
AU - Gladstone,GR
AU - Retherford,KD
AU - Dougherty,MK
AU - Wahlund,J-E
AU - Barabash,S
AU - Iess,L
AU - Bruzzone,L
AU - Hussmann,H
AU - Gurvits,LI
AU - Santolik,O
AU - Kolmasova,I
AU - Fischer,G
AU - Müller-Wodarg,I
AU - Piccioni,G
AU - Fouchet,T
AU - Gérard,J-C
AU - Sánchez-Lavega,A
AU - Irwin,PGJ
AU - Grodent,D
AU - Altieri,F
AU - Mura,A
AU - Drossart,P
AU - Kammer,J
AU - Giles,R
AU - Cazaux,S
AU - Jones,G
AU - Smirnova,M
AU - Lellouch,E
AU - Medvedev,AS
AU - Moreno,R
AU - Rezac,L
AU - Coustenis,A
AU - Costa,M
DO - 10.1007/s11214-023-00996-6
PY - 2023///
SN - 0038-6308
TI - Jupiter science Enabled by ESA's Jupiter Icy Moons Explorer
T2 - Space Science Reviews
UR - http://dx.doi.org/10.1007/s11214-023-00996-6
UR - https://www.ncbi.nlm.nih.gov/pubmed/37744214
UR - https://link.springer.com/article/10.1007/s11214-023-00996-6
UR - http://hdl.handle.net/10044/1/106830
VL - 219
ER -
