activity
20132021
most citedThe Influence of Spatial Resolution on Nonlinear Force-Free Modeling

87 citations · 185 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2021★ 20 cited

Magnetic helicity estimations in models and observations of the solar magnetic field. Part IV: Application to solar observations

J. K. Thalmann, M. K. Georgoulis, Y. Liu +8

In this ISSI-supported series of studies on magnetic helicity in the Sun, we systematically implement different magnetic helicity calculation methods on high-quality solar magnetog…

astro-ph.SR2017★ 20 cited

The causes of quasi-homologous CMEs

Lijuan Liu, Yuming Wang, Rui Liu +8

In this paper, we identified the magnetic source locations of 142 quasi- homologous (QH) coronal mass ejections (CMEs), of which 121 are from solar cycle (SC) 23 and 21 from SC 24.…

astro-ph.SR2016★ 12 cited

Arcade Implosion Caused by a Filament Eruption in a Flare

Juntao Wang, P. J. A. Simoes, L. Fletcher +3

Coronal implosions - the convergence motion of plasmas and entrained magnetic field in the corona due to a reduction in magnetic pressure - can help to locate and track sites of ma…

astro-ph.SR2016★ 6 cited

Temporal and spatial relationship of flare signatures and the force-free coronal magnetic field

Julia K. Thalmann, Astrid M. Veronig, Yang Su

We investigate the plasma and magnetic environment of active region NOAA 11261 on 2 August 2011 around a GOES M1.4 flare/CME (SOL2011-08-02T06:19). We compare coronal emission at (…

astro-ph.SR2015★ 87 cited

The Influence of Spatial Resolution on Nonlinear Force-Free Modeling

M. L. DeRosa, M. S. Wheatland, K. D. Leka +11

The nonlinear force-free field (NLFFF) model is often used to describe the solar coronal magnetic field, however a series of earlier studies revealed difficulties in the numerical…

astro-ph.SR2013★ 40 cited

Force-free field modeling of twist and braiding-induced magnetic energy in an active-region corona

J. K. Thalmann, S. K. Tiwari, T. Wiegelmann

The theoretical concept that braided magnetic field lines in the solar corona may dissipate a sufficient amount of energy to account for the brightening observed in the active-regi…