305 citations · 2.5k across the 47 of their papers we have counts for
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Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection
C. J. Schrijver, M. L. DeRosa, T. Metcalf +14
Solar flares and coronal mass ejections are associated with rapid changes in field connectivity and powered by the partial dissipation of electrical currents in the solar atmospher…
Are constant loop widths an artifact of the background and the spatial resolution?
M. C. Lopez Fuentes, P. Demoulin, J. A. Klimchuk
We study the effect of the coronal background in the determination of the diameter of EUV loops, and we analyze the suitability of the procedure followed in a previous paper (López…
Eruption of a Kink-Unstable Filament in Active Region NOAA 10696
D. R. Williams, T. Toeroek, P. Demoulin +2
We present rapid-cadence Transition Region And Coronal Explorer (TRACE) observations which show evidence of a filament eruption from active region NOAA 10696, accompanied by an X2.…
The Magnetic Structure of Coronal Loops Observed by TRACE
M. C. Lopez Fuentes, J. A. Klimchuk, P. Demoulin
Previous studies have found that coronal loops have a nearly uniform thickness, which seems to disagree with the characteristic expansion of active region magnetic fields. This is…
Quasi-Separatrix Layers: Refined Theory and its Application to Solar Flares
V. S. Titov, P. Demoulin, G. Hornig
Although the analysis of observational data indicates that quasi-separatrix layers (QSLs) have to play an important role in magnetic configurations of solar flares, the correspondi…