Evolution of the magnetic flux around a solar flare associated with a filament eruption
Abstract
Using a nonlinear force-free field (NLFFF) algorithm, we calculated the magnetic flux around M3.7 class solar flare produced by Active Region 13229 (AR 13229), located in the northern solar hemisphere (N29W24), on February 24, 2023. The solar flare is associated with a filament eruption, and these phenomena produced a coronal mass ejection with an earth-directed component. Also, we obtained the 3D magnetic configuration from photospheric magnetic magnetograms Space Weather HMI Active Region Patch (SHARP) from the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO).
- Publication:
-
7th International Conference in Astronomy
- Pub Date:
- July 2023
- Bibcode:
- 2023aasp.confE..26D