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ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailedinvestigation of the Jovian system in the 2030s, combining a suite ofstate-of-the-art instruments with an orbital tour tailored to maximiseobserving opportunities. We review the Jupiter science enabled by the JUICEmission, building on the legacy of discoveries from the Galileo, Cassini, andJuno missions, alongside ground- and space-based observatories. We focus onremote sensing of the climate, meteorology, and chemistry of the atmosphere andauroras from the cloud-forming weather layer, through the upper troposphere,into the stratosphere and ionosphere. The Jupiter orbital tour provides awealth of opportunities for atmospheric and auroral science: globalperspectives with its near-equatorial and inclined phases, sampling all phaseangles from dayside to nightside, and investigating phenomena evolving ontimescales from minutes to months. The remote sensing payload spans far-UVspectroscopy (50-210 nm), visible imaging (340-1080 nm), visible/near-infraredspectroscopy (0.49-5.56 $\mu$m), and sub-millimetre sounding (near 530-625\,GHzand 1067-1275\,GHz). This is coupled to radio, stellar, and solar occultationopportunities to explore the atmosphere at high vertical resolution; and radioand plasma wave measurements of electric discharges in the Jovian atmosphereand auroras. Cross-disciplinary scientific investigations enable JUICE toexplore coupling processes in giant planet atmospheres, to show how theatmosphere is connected to (i) the deep circulation and composition of thehydrogen-dominated interior; and (ii) to the currents and charged particleenvironments of the external magnetosphere. JUICE will provide a comprehensivecharacterisation of the atmosphere and auroras of this archetypal giant planet.

Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer