Coronal Models and Detection of the Open Magnetic Field

Bibliographic Details
Title: Coronal Models and Detection of the Open Magnetic Field
Authors: Eleanna Asvestari, Manuela Temmer, Ronald M. Caplan, Jon A. Linker, Stephan G. Heinemann, Rui F. Pinto, Carl J. Henney, Charles N. Arge, Mathew J. Owens, Maria S. Madjarska, Jens Pomoell, Stefan J. Hofmeister, Camilla Scolini, Evangelia Samara
Source: The Astrophysical Journal, Vol 971, Iss 1, p 45 (2024)
Publisher Information: IOP Publishing, 2024.
Publication Year: 2024
Collection: LCC:Astrophysics
Subject Terms: Solar corona, Solar magnetic fields, Solar physics, Solar coronal holes, Solar active regions, Magnetohydrodynamics, Astrophysics, QB460-466
More Details: A plethora of coronal models, from empirical to more complex magnetohydrodynamic (MHD) ones, are being used for reconstructing the coronal magnetic field topology and estimating the open magnetic flux. However, no individual solution fully agrees with coronal hole observations and in situ measurements of open flux at 1 au, as there is a strong deficit between the model and observations contributing to the known problem of the missing open flux. In this paper, we investigate the possible origin of the discrepancy between modeled and observed magnetic field topology by assessing the effect on the simulation output by the choice of the input boundary conditions and the simulation setup, including the choice of numerical schemes and the parameter initialization. In the frame of this work, we considered four potential field source surface-based models and one fully MHD model, different types of global magnetic field maps, and model initiation parameters. After assessing the model outputs using a variety of metrics, we conclude that they are highly comparable regardless of the differences set at initiation. When comparing all models to coronal hole boundaries extracted by extreme-ultraviolet filtergrams, we find that they do not compare well. This mismatch between observed and modeled regions of the open field is a candidate contributing to the open flux problem.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1538-4357
Relation: https://doaj.org/toc/1538-4357
DOI: 10.3847/1538-4357/ad5155
Access URL: https://doaj.org/article/ac2f1e1828064f5db476d94c8df92686
Accession Number: edsdoj.2f1e1828064f5db476d94c8df92686
Database: Directory of Open Access Journals
More Details
ISSN:15384357
DOI:10.3847/1538-4357/ad5155
Published in:The Astrophysical Journal
Language:English