Add to ORKGAbstract. MHD simulation is performed in the corona above the active region AR 0365 before the series of flares 26 and 27 May 2003. The special methods are developed which permit to set all conditions for MHD equations from observations. The behavior of the magnetic field and plasma near current sheets appeared in the corona is studied
We present the results of a set of three-dimensional numerical simulations of magnetic flux emergenc...
Using ideal and resistive MHD, we investigate the stability and dynamic evolution of three-dimension...
Magnetohydrodynamic (MHD) processes are important for the transfer of energy over large scales in pl...
Abstract. New observations justify the flare scenario predicted by the electrodynamical model based ...
Temporal evolution of a current sheet with initial perturbations is studied by using the three-dimen...
The magnetohydrodynamic (MHD) simulations are often used in problems solved both in low- and high-te...
Context. Active region (AR) 8210 was the host of many flares and coronal mass ejections (CMEs). Stud...
Abstract—New data for the energy and location of the hard-emission centers of a solar flare agree wi...
We perform MHD modeling of a single bright coronal loop to include the interaction with a non-unifor...
Coronal mass ejections (CMEs) and solar flares are the main drivers of weather in space. Understandi...
Aims: Solar photospheric footpoint motions can produce strong, localised currents in the corona. A d...
Aims. Solar photospheric footpoint motions can produce strong, localised currents in the corona. A d...
The interaction phase of the Converging Flux Model (Priest ct al., 1994) for the formation of corona...
We present the results of a set of three-dimensional numerical simulations of magnetic flux emergenc...
Context. The data-driven and time-dependent modeling of coronal magnetic fields is crucial for under...
We present the results of a set of three-dimensional numerical simulations of magnetic flux emergenc...
Using ideal and resistive MHD, we investigate the stability and dynamic evolution of three-dimension...
Magnetohydrodynamic (MHD) processes are important for the transfer of energy over large scales in pl...
Abstract. New observations justify the flare scenario predicted by the electrodynamical model based ...
Temporal evolution of a current sheet with initial perturbations is studied by using the three-dimen...
The magnetohydrodynamic (MHD) simulations are often used in problems solved both in low- and high-te...
Context. Active region (AR) 8210 was the host of many flares and coronal mass ejections (CMEs). Stud...
Abstract—New data for the energy and location of the hard-emission centers of a solar flare agree wi...
We perform MHD modeling of a single bright coronal loop to include the interaction with a non-unifor...
Coronal mass ejections (CMEs) and solar flares are the main drivers of weather in space. Understandi...
Aims: Solar photospheric footpoint motions can produce strong, localised currents in the corona. A d...
Aims. Solar photospheric footpoint motions can produce strong, localised currents in the corona. A d...
The interaction phase of the Converging Flux Model (Priest ct al., 1994) for the formation of corona...
We present the results of a set of three-dimensional numerical simulations of magnetic flux emergenc...
Context. The data-driven and time-dependent modeling of coronal magnetic fields is crucial for under...
We present the results of a set of three-dimensional numerical simulations of magnetic flux emergenc...
Using ideal and resistive MHD, we investigate the stability and dynamic evolution of three-dimension...
Magnetohydrodynamic (MHD) processes are important for the transfer of energy over large scales in pl...