P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona

P-CORONA: A New Tool for Calculating the Intensity and Polarization of Coronal Lines in 3D Models of the Solar Corona

The critical need to study the magnetic field in the solar corona is highlighted by recent observational facilities, such as the Daniel K. Inouye Solar Telescope and Aditya-L1. A powerful tool for probing the magnetism of the solar corona is forward modeling of the intensity and polarization of coro...

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Bibliographic Details
Main Authors: Supriya Hebbur Dayananda, Ángel de Vicente, Tanausú del Pino Alemán, Javier Trujillo Bueno, Nataliia G. Shchukina
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar corona
Solar magnetic fields
Solar coronal lines
Solar physics
Spectropolarimetry
Online Access:https://doi.org/10.3847/1538-4357/add32e
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https://doi.org/10.3847/1538-4357/add32e

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