24 citations · 33 across the 6 of their papers we have counts for
6 papers
Activity of low mass stars in the light of spot signature in the Fourier domain
Lucie Degott, Frederic Baudin, Reza Samadi +2
Context. Magnetic fields exhibit a wide variety of behaviours in low mass stars and further characterization is required to understand these observations. Stellar photometry from s…
How coronal mass ejections are influenced by the morphology and toroidal flux of their source magnetic flux ropes?
J. H. Guo, L. Linan, S. Poedts +9
Coronal mass ejections (CMEs) stand as intense eruptions of magnetized plasma from the Sun, playing a pivotal role in driving significant changes of the heliospheric environment. D…
Modelling the propagation of coronal mass ejections with COCONUT: implementation of the Regularized Biot-Savart Laws flux rope model
Jinhan Guo, L. Linan, S. Poedts +8
Context: Coronal mass ejections (CMEs) are rapid eruptions of magnetized plasma that occur on the Sun, which are known as the main drivers of adverse space weather. Accurately trac…
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…
Assessing inner boundary conditions for global coronal modeling of solar maxima
Michaela Brchnelova, Błażej Kuźma, Fan Zhang +3
Computational Fluid Dynamics (CFD)-based global solar coronal simulations are slowly making their way into the space weather modeling toolchains to replace the semi-empirical metho…
Spontaneous flux concentrations from the negative effective magnetic pressure instability beneath a radiative stellar surface
Barbara Perri, Axel Brandenburg
The formation of sunspots requires the concentration of magnetic flux near the surface. The negative magnetic pressure instability (NEMPI) might be a possible mechanism for accompl…