activity
20082022
most citedDeriving the radial distances of wide coronal mass ejections from elongation measurements in the heliosphere - Application to CME-CME interaction

169 citations · 582 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2022★ 6 cited

Modelling the magnetic structure of a large-scale horse-shoe-like filament in a decaying and diffuse active region

Kaifeng Kang, Yang Guo, Ilia I. Roussev +2

A large-scale, horse-shoe-like filament was investigated and the magnetic field around it was reconstructed. This is an intermediate filament (IF) that appeared on the solar disk f…

astro-ph.SR2019★ 13 cited

Evolution of CME Properties in the Inner Heliosphere: Prediction for Solar Orbiter and Parker Solar Probe

Nada Al-Haddad, Noe Lugaz, Stefaan Poedts +2

The evolution of the magnetic field and plasma quantities inside a coronal mass ejection (CME) with distance are known from statistical studies using data from 1 au monitors, plane…

astro-ph.SR2013★ 52 cited

Impact of Temperature-dependent resistivity and thermal conduction on plasmoid Instabilities in current sheets in the solar corona

Lei Ni, Ilia I. Roussev, Jun Lin +1

In this paper we investigate, by means of two-dimensional magnetohydrodynamic simulations, the impact of temperature-dependent resistivity and thermal conduction on the development…

astro-ph.SR2012★ 83 cited

Magnetic Field Configuration Models and Reconstruction Methods for Interplanetary Coronal Mass Ejections

N. Al-Haddad, T. Nieves-Chinchilla, N. P. Savani +6

This study aims to provide a reference to different magnetic field models and reconstruction methods for interplanetary coronal mass ejections (ICMEs). In order to understand the d…

astro-ph.SR2011★ 116 cited

Numerical Investigation of a Coronal Mass Ejection from an Anemone Active Region: Reconnection and Deflection of the 2005 August 22 Eruption

N. Lugaz, C. Downs, K. Shibata +3

We present a numerical investigation of the coronal evolution of a coronal mass ejection (CME) on 2005 August 22 using a 3-D thermodynamics magnetohydrodynamic model, the SWMF. The…

astro-ph.SR2010★ 128 cited

Determining the azimuthal properties of coronal mass ejections from multi-spacecraft remote-sensing observations with stereo secchi

N. Lugaz, J. N. Hernandez-Charpak, I. I. Roussev +3

We discuss how simultaneous observations by multiple heliospheric imagers can provide some important information about the azimuthal properties of Coronal Mass Ejections (CMEs) in…