Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT

Wang, Haipeng; Poedts, Stefaan; Lani, Andrea; Linan, L.; Baratashvili, Tinatin; Zhang, Fan; Sorokina, D.; Jeong, H.T.; Li, Yuchuan; Najafi-Ziyazi, Mahdi; Schmieder, B.

doi:10.1051/0004-6361/202555760

Public

Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT

Shared by NobleBlocks on Aug 20, 2025 • 12:00 AM UTC

Authors:

Haipeng Wang

Stefaan Poedts

Andrea Lani

Abstract

Context. Time-evolving magnetohydrodynamic (MHD) coronal models driven by a sequence of time-evolving photospheric magnetograms deliver more realistic results than traditional quasi-steady-state models constrained by a static magnetogram. The fully implicit time-evolving coronal model COCONUT perfor...

Subject

Physics

Astrophysics

Astronomy

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