Showing 1–20 of 25 results
/ Date/ Name
Jun 27, 2017The causes of quasi-homologous CMEsFeb 5, 2016Chromospheric evaporation flows and density changes deduced from Hinode/EIS during an M1.6 flareJul 12, 2007Large amplitude oscillatory motion along a solar filamentJan 17, 2008Can We Improve the Preprocessing of Photospheric Vector Magnetograms by the Inclusion of Chromospheric Observations?Jan 18, 2008Preprocessing of Hinode/SOT vector magnetograms for nonlinear force-free coronal magnetic field modellingNov 30, 2007Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejectionSep 25, 2013Twisting solar coronal jet launched at the boundary of an active regionJun 6, 2012Nonlinear force-free field modeling of a solar active region using SDO/HMI and SOLIS/VSM dataFeb 18, 2015The Confined X-class Flares of Solar Active Region 2192Aug 22, 2015The Influence of Spatial Resolution on Nonlinear Force-Free ModelingDec 21, 2023On the use of relative field line helicity as an indicator for solar eruptivityJun 16, 2021Magnetic helicity and energy budget around large confined and eruptive solar flaresApr 20, 2022The effect of spatial sampling on magnetic field modeling and helicity computationOct 15, 2019Magnetic helicity budget of solar active regions prolific of eruptive and confined flaresFeb 19, 2024Stability of the coronal magnetic field around large confined and eruptive solar flaresMar 2, 2017On flare-CME characteristics from Sun to Earth combining remote-sensing image data with in-situ measurements supported by modelingApr 12, 2013Comparison of force-free coronal magnetic field modeling using vector fields from Hinode and Solar Dynamics ObservatoryOct 19, 2016Arcade Implosion Caused by a Filament Eruption in a FlareNov 14, 2013Force-free field modeling of twist and braiding-induced magnetic energy in an active-region coronaApr 7, 2017Magnetic Helicity Estimations in Models and Observations of the Solar Magnetic Field. Part III: Twist Number Method