Publications (20)
Eruption of a Kink-Unstable Filament in Active Region NOAA 10696
D. R. Williams, T. Toeroek, P. Demoulin +2
Magnetic Reconnection along Quasi-Separatrix Layers as a Driver of Ubiquitous Active Region Outflows
D. Baker, L. van Driel-Gesztelyi, C. H. Mandrini +2
In Situ Properties of Small and Large Flux Ropes in the Solar Wind
M. Janvier, P. Demoulin, S. Dasso
Why are flare ribbons associated with the spines of magnetic null points generically elongated?
D. I. Pontin, K. Galsgaard, P. Demoulin
The standard flare model in three dimensions. II. Upper limit on solar flare energy
G. Aulanier, P. Demoulin, C. J. Schrijver +3
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
Criteria for Flux Rope Eruption: Non Equilibrium versus Torus Instability
P. Demoulin, G. Aulanier
Signatures of Interchange Reconnection: STEREO, ACE and Hinode Observations Combined
D. Baker, A. P. Rouillard, L. van Driel-Gesztelyi +8
Magnetic Flux and Helicity of Magnetic Clouds
P. Demoulin, M. Janvier, S. Dasso
Accuracy of magnetic energy computations
G. Valori, P. Demoulin, E. Pariat +1
Coronal magnetic reconnection driven by CME expansion -- the 2011 June 7 event
L. van Driel-Gesztelyi, D. Baker, T. Torok +10
How are Emerging Flux, Flares and CMEs Related to Magnetic Polarity Imbalance in MDI Data?
L. M. Green, P. Demoulin, C. H. Mandrini +1
Tracking Solar Active Region Outflow Plasma from its Source to the near-Earth Environment
J. L. Culhane, D. H. Brooks, L. van Driel-Gesztelyi +6
The Magnetic Structure of Coronal Loops Observed by TRACE
M. C. Lopez Fuentes, J. A. Klimchuk, P. Demoulin
The 3D geometry of active region upflows deduced from their limb-to-limb evolution
P. Demoulin, D. Baker, C. H. Mandrini +1
Quasi-Separatrix Layers: Refined Theory and its Application to Solar Flares
V. S. Titov, P. Demoulin, G. Hornig
Plasma composition in a sigmoidal anemone active region
D. Baker, D. H. Brooks, P. Demoulin +4
Solar filament eruptions and their physical role in triggering Coronal Mass Ejections
B. Schmieder, P. Demoulin, G. Aulanier
Are constant loop widths an artifact of the background and the spatial resolution?
M. C. Lopez Fuentes, P. Demoulin, J. A. Klimchuk
Does the spacecraft trajectory strongly affect the detection of magnetic clouds?
P. Demoulin, S. Dasso, M. Janvier