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More model informationExplore the intricate magnetic field dynamics within the HD189733A system. Hosting a hot Jupiter subjected to intense stellar irradiation, the planetary outflow undergoes significant perturbations due to interaction with the stellar wind. This interaction results in noteworthy reconnection phenomena, altering the overall magnetic field configuration of the system.
We acknowledge PRACE for awarding access to the Fenix Infrastructure resources at CINECA, which are partially funded from the European Union’s Horizon 2020 research and innovation programme through the ICEI project under the grant agreement No. 800858.
CC AttributionCreative Commons Attribution
Dec 7th 2023
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