Publications (18)
Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope
Deborah Baker, Teodora Mihailescu, Pascal Demoulin +6
One of the major discoveries of Hinode's Extreme-ultraviolet Imaging Spectrometer (EIS) is the presence of upflows at the edges of active regions. As active regions are magneticall…
Understanding CME and associated shock in the solar corona by merging multi wavelengths observation
Pietro Zucca, Monique Pick, Pascal Demoulin +3
Using multi-wavelength imaging observations, in EUV, white light and radio, and radio spectral data over a large frequency range, we analyzed the triggering and development of a co…
From coronal observations to MHD simulations, the building blocks for 3D models of solar flares
Miho Janvier, Guillaume Aulanier, Pascal Demoulin
Solar flares are energetic events taking place in the Sun's atmosphere, and their effects can greatly impact the environment of the surrounding planets. In particular, eruptive fla…
Counter-Streaming Velocities in a Quiescent Filament
Garima Karki, Brigitte Schmieder, Pascal Demoulin +3
Filaments/prominences are cold plasma (~ 10000 K) embedded in the solar corona, two orders of magnitude hotter. Filament plasma is structured by the magnetic field in thin elongate…
Comparing generic models for interplanetary shocks and magnetic clouds axis configurations at 1 AU
Miho Janvier, Sergio Dasso, Pascal Demoulin +2
Interplanetary Coronal Mass Ejections are the manifestation of solar transient eruptions, which can significantly modify the plasma and magnetic conditions in the heliosphere. They…
Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation
Miho Janvier, Pascal Demoulin, Sergio Dasso
Coronal mass ejections (CMEs) are routinely tracked with imagers in the interplanetary space while magnetic clouds (MCs) properties are measured locally by spacecraft. However, bot…