activity
20072009
most citedNon-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection

305 citations · 484 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR200965 cited

A self-consistent nonlinear force-free solution for a solar active region magnetic field

M. S. Wheatland, S. Regnier

Nonlinear force-free solutions for the magnetic field in the solar corona constructed using photospheric vector magnetic field boundary data suffer from a basic problem: the observ…

astro-ph.SR20098 cited

Relationship between photospheric currents and coronal magnetic helicity for force-free bipolar fields

S. Regnier

The origin and evolution of the magnetic helicity in the solar corona are not well understood. For instance, the magnetic helicity of an active region is often about Mx$^…

astro-ph200823 cited

Coronal Alfven speeds in an isothermal atmosphere I. Global properties

S. Regnier, E. R. Priest, A. W. Hood

Estimating Alfven speeds is of interest in modelling the solar corona, studying the coronal heating problem and understanding the initiation and propagation of coronal mass ejectio…

astro-ph200827 cited

POLAR Investigation of the Sun - POLARIS

T. Appourchaux, P. Liewer, M. Watt +34

The POLAR Investigation of the Sun (POLARIS) mission uses a combination of a gravity assist and solar sail propulsion to place a spacecraft in a 0.48 AU circular orbit around the S…

astro-ph2007305 cited

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…

astro-ph200756 cited

Nonlinear force-free models for the solar corona I. Two active regions with very different structure

S. Regnier, E. R. Priest

With the development of new instrumentation providing measurements of solar photospheric vector magnetic fields, we need to develop our understanding of the effects of current dens…