Data-driven, time-dependent modeling of pre-eruptive coronal magnetic field configuration at the periphery of NOAA AR 11726-Reference-Cited by-同舟云学术

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Data-driven, time-dependent modeling of pre-eruptive coronal magnetic field configuration at the periphery of NOAA AR 11726

Published:2021-09-27 Issue: Volume: Page:
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Lumme E.,Pomoell J.,Price D. J.,Kilpua E. K. J.,Kazachenko M. D.,Fisher G. H.,Welsch B. T.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://www.aanda.org/10.1051/0004-6361/202038744/pdf

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1. Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropes;Reviews of Modern Plasma Physics;2024-08-10

2. The winding number of coronal flux ropes;Astronomy & Astrophysics;2024-06

3. Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions;The Astrophysical Journal Supplement Series;2024-02-01

4. A Near-half-century Simulation of the Solar Corona;The Astrophysical Journal Letters;2024-01-01

5. Hybrid Data-driven Magnetofrictional and Magnetohydrodynamic Simulations of an Eruptive Solar Active Region;The Astrophysical Journal;2023-07-24

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