112 citations · 2.9k across the 157 of their papers we have counts for
6 papers · 1 filter
Constraints for the aperiodic O-mode streaming instability
M. Lazar, R. Schlickeiser, S. Poedts +2
In plasmas where the thermal energy density exceeds the magnetic energy density (), the aperiodic ordinary mode (O-mode) instability is driven by an excess of para…
Observational Characteristics of CMEs without Low Coronal Signatures
E. D'Huys, D. B. Seaton, S. Poedts +1
Solar eruptions are usually associated with a variety of phenomena occurring in the low corona before, during, and after onset of eruption. Though easily visible in coronagraph obs…
Simulating AIA observations of a flux rope ejection
Paolo Pagano, Duncan H. Mackay, Stefaan Poedts
Extreme ultraviolet (EUV) images from the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory (SDO) are providing new insights into the early phase of CME evo…
Overstability of acoustic waves in strongly magnetized anisotropic MHD shear flows
E. S. Uchava, B. M. Shergelashvili, A. G. Tevzadze +1
We present a linear stability analysis of the perturbation modes in anisotropic MHD flows with velocity shear and strong magnetic field. Collisionless or weakly collisional plasma…
Solar Wind Electron Strahls Associated with a High-Latitude CME: \emph{Ulysses} Observations
M. Lazar, J. Pomoell, S. Poedts +2
Counterstreaming beams of electrons are ubiquitous in coronal mass ejections (CMEs) - although their existence is not unanimously accepted as a necessary and/or sufficient signatur…
Observational evidence of torus instability as trigger mechanism for coronal mass ejections: the 2011 August 4 filament eruption
Francesco P. Zuccarello, Daniel B. Seaton, Marilena Mierla +4
Solar filaments are magnetic structures often observed in the solar atmosphere and consist of plasma that is cooler and denser than their surroundings. They are visible for days --…