The Bright Rim Prominences according to 2.5D Radiative Transfer

Solar prominences observed close to the limb commonly include a bright feature that, from the perspective of the observer, runs along the interface between itself and the underlying chromosphere. Despite several idealized models being proposed to explain the underlying physics, a more general approa...

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Bibliographic Details

Published in:	The Astrophysical Journal Letters
Main Authors:	Jack M. Jenkins, Christopher M. J. Osborne, Ye Qiu, Rony Keppens, Chuan Li
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Solar prominences Solar filaments Radiative transfer Solar chromosphere
Online Access:	https://doi.org/10.3847/2041-8213/ad3423