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Two-horn quiescent prominence observed in H-alpha and MgII h&k lines with THEMIS and IRIS
Krzysztof Barczynski, Brigitte Schmieder, Bernard Gelly +2
Prominences are large magnetic structures in the corona filled by cool plasma with fast evolving fine structure. We aim to better understand the plasma conditions in the fine struc…
Understanding the Lateral Drifting of an Erupting Filament with a Data-constrained Magnetohydrodynamic Simulation
Jinhan Guo, Ye Qiu, Yiwei Ni +6
Solar filaments often exhibit rotation and deflection during eruptions, which would significantly affect the geoeffectiveness of the corresponding coronal mass ejections (CMEs). Th…
Impact of the solar activity on the propagation of ICMEs: Simulations of hydro, magnetic and median ICMEs at minimum and maximum of activity
Barbara Perri, Brigitte Schmieder, Pascal Démoulin +2
The propagation of Interplanetary Coronal Mass Ejections (ICMEs) in the heliosphere is influenced by many physical phenomena, related to the internal structure of the ICME and its…
Rotation and interaction of the September 8 and 10, 2014 CMEs tested with EUHFORIA
Anwesha Maharana, Camilla Scolini, Brigitte Schmieder +1
Solar coronal mass ejections (CMEs) can catch up and interact with preceding CMEs and solar wind structures to undergo rotation and deflection during their propagation. We aim to s…
Self-consistent propagation of flux ropes in realistic coronal simulations
L. Linan, F. Regnault, B. Perri +5
The aim of this paper is to demonstrate the possible use of the new coronal model COCONUT to compute a detailed representation of a numerical CME at 0.1~AU, after its injection at…
Simulation of a Solar Jet Formed from an Untwisting Flux Rope Interacting with a Null Point
Jiahao Zhu, Yang Guo, Mingde Ding +1
Coronal jets are eruptions identified by a collimated, sometimes twisted spire. They are small-scale energetic events compared with flares. Using multi-wavelength observations from…