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Modeling of the exoplanet HAT-P-11b magnetosphere
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Based on the available data on the magnetic field of the star HAT-P-11 and its closest exoplanet HAT-P-11b, as well as information on the stellar wind in this system, we construct the HAT-P-11b magnetic field magnetospheric model. We show how the value and orientation of the interplanetary magnetic field control the magnetospheric structure. Each component of the stellar wind’s magnetic field creates a specific type of reconnection with the exoplanet’s magnetic field.
The Russian Academy of Sciences
Title: Modeling of the exoplanet HAT-P-11b magnetosphere
Description:
Based on the available data on the magnetic field of the star HAT-P-11 and its closest exoplanet HAT-P-11b, as well as information on the stellar wind in this system, we construct the HAT-P-11b magnetic field magnetospheric model.
We show how the value and orientation of the interplanetary magnetic field control the magnetospheric structure.
Each component of the stellar wind’s magnetic field creates a specific type of reconnection with the exoplanet’s magnetic field.
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