We report on three-dimensional (3D) MHD simulations of recurrent mini CME-like eruptions in a small active region (AR), which is formed by the dynamical emergence of a twisted (not kink unstable) flux tube from the solar interior. The eruptions are developed as a result of repeated formation and expulsion of new flux ropes due to continous emergence and reconnection of sheared fieldlines along the polarity inversion line (PIL) of the AR. The acceleration of the eruptions is triggered by tether-cutting reconnection at the current sheet underneath the erupting field. We find that each explosive eruption is followed by reformation of a sigmoidal structure and a subsequent “sigmoid-to-flare arcade ” transformation in the AR. These results might...
We present results of three-dimensional MHD simulations of recurrent eruptions in emerging flux regi...
Large-scale solar eruptions, known as coronal mass ejections (CMEs), are regarded as the main driver...
We present results of three-dimensional MHD simulations of recurrent eruptions in emerging flux regi...
We report on three-dimensional MHD simulations of recurrent mini coronal mass ejection (CME)-like er...
We report on three-dimensional MHD simulations of recurrent mini coronal mass ejection (CME)-like er...
The authors acknowledge support by EU (IEF-272549 grant) and the Royal Society.We report on three-di...
We report on three-dimensional (3D) magnetohydrodynamic (MHD) simulations of recurrent eruptions in ...
This project has received funding from the Science and Technology Facilities Council (UK) through th...
An eruption event launched from solar active region (AR) NOAA 11719 is investigated based on coronal...
We have simulated the three-dimensional (3D) emergence and interaction of two twisted flux tubes, wh...
Solar eruptions are the most energetic phenomena observed in the solar system observed as flares, co...
Abstract We study a filament eruption, two-ribbon flare, and coronal mass ejection (CME) that occurr...
Solar eruptions are often generated as a result of the complex magnetic environment in solar active ...
Solar eruptions are often generated as a result of the complex magnetic environment in solar active ...
Coronal mass ejections (CMEs) erupt and expand in a magnetically structured solar corona. Various in...
We present results of three-dimensional MHD simulations of recurrent eruptions in emerging flux regi...
Large-scale solar eruptions, known as coronal mass ejections (CMEs), are regarded as the main driver...
We present results of three-dimensional MHD simulations of recurrent eruptions in emerging flux regi...
We report on three-dimensional MHD simulations of recurrent mini coronal mass ejection (CME)-like er...
We report on three-dimensional MHD simulations of recurrent mini coronal mass ejection (CME)-like er...
The authors acknowledge support by EU (IEF-272549 grant) and the Royal Society.We report on three-di...
We report on three-dimensional (3D) magnetohydrodynamic (MHD) simulations of recurrent eruptions in ...
This project has received funding from the Science and Technology Facilities Council (UK) through th...
An eruption event launched from solar active region (AR) NOAA 11719 is investigated based on coronal...
We have simulated the three-dimensional (3D) emergence and interaction of two twisted flux tubes, wh...
Solar eruptions are the most energetic phenomena observed in the solar system observed as flares, co...
Abstract We study a filament eruption, two-ribbon flare, and coronal mass ejection (CME) that occurr...
Solar eruptions are often generated as a result of the complex magnetic environment in solar active ...
Solar eruptions are often generated as a result of the complex magnetic environment in solar active ...
Coronal mass ejections (CMEs) erupt and expand in a magnetically structured solar corona. Various in...
We present results of three-dimensional MHD simulations of recurrent eruptions in emerging flux regi...
Large-scale solar eruptions, known as coronal mass ejections (CMEs), are regarded as the main driver...
We present results of three-dimensional MHD simulations of recurrent eruptions in emerging flux regi...