During this period of performance (1 Jan. 1992 - 31 Dec. 1992), the investigation of the following tasks was accomplished: (1) application of the Non-linear Force-free Field (NLFF) Model to study the active region evolution; (2) coronal dynamical responses due to emerging flux including the transition region; (3) loss of MHD equilibrium due to footpoint motions; and (4) two-dimensional MHD global coronal model: steady-state streamers. The detailed description of these studies are included
We present observations and modeling of the magnetic field configuration, morphology, and dynamics o...
We examine how the initial state (pre-event corona) affects the numerical MHD simulation for a coron...
The coronal magnetic field evolution of 20 bipolar active regions (ARs) is simulated from their emer...
Papers covering the following topics are presented: flare physics; coronal dynamics; interplanetary ...
International audienceIn this paper we show that when accurate nonlinear force-free field (NLFFF) mo...
Context. The data-driven and time-dependent modeling of coronal magnetic fields is crucial for under...
Context. Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the Sun...
Throughout the eleven year cycle of the sun, solar eruptions are constantly taking place. Thought to...
Coronal mass ejections (CMEs) and solar flares are the main drivers of weather in space. Understandi...
Funding: STFC via the Consolidated Grant SMC1/YST025 (SLY), STFC and the Levehulme Trust (DHM).The c...
Nonlinear force-free field (NLFFF) models are thought to be viable tools for investigating the struc...
International audienceWe study the magnetic structure of successively erupting sigmoid in active reg...
The coronal magnetic field evolution of 20 bipolar active regions (ARs) is simulated from their emer...
Context. Coronal mass ejections (CMEs) that exhibit weak or no eruption signatures in the low corona...
The response of coronal magnetic fields to photospheric motion is investigated using a time-dependen...
We present observations and modeling of the magnetic field configuration, morphology, and dynamics o...
We examine how the initial state (pre-event corona) affects the numerical MHD simulation for a coron...
The coronal magnetic field evolution of 20 bipolar active regions (ARs) is simulated from their emer...
Papers covering the following topics are presented: flare physics; coronal dynamics; interplanetary ...
International audienceIn this paper we show that when accurate nonlinear force-free field (NLFFF) mo...
Context. The data-driven and time-dependent modeling of coronal magnetic fields is crucial for under...
Context. Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the Sun...
Throughout the eleven year cycle of the sun, solar eruptions are constantly taking place. Thought to...
Coronal mass ejections (CMEs) and solar flares are the main drivers of weather in space. Understandi...
Funding: STFC via the Consolidated Grant SMC1/YST025 (SLY), STFC and the Levehulme Trust (DHM).The c...
Nonlinear force-free field (NLFFF) models are thought to be viable tools for investigating the struc...
International audienceWe study the magnetic structure of successively erupting sigmoid in active reg...
The coronal magnetic field evolution of 20 bipolar active regions (ARs) is simulated from their emer...
Context. Coronal mass ejections (CMEs) that exhibit weak or no eruption signatures in the low corona...
The response of coronal magnetic fields to photospheric motion is investigated using a time-dependen...
We present observations and modeling of the magnetic field configuration, morphology, and dynamics o...
We examine how the initial state (pre-event corona) affects the numerical MHD simulation for a coron...
The coronal magnetic field evolution of 20 bipolar active regions (ARs) is simulated from their emer...