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astro-ph.SR2024
Magnetic evolution of active regions: formation and eruption of magnetic flux ropes
P. Vemareddy
Magnetic flux ropes (FRs) are twisted structures appearing on the sun, predominantly in the magnetically concentrated regions. These structures appear as coronal features known as…
astro-ph.SR2024
Simulating the formation and eruption of flux rope by magneto-friction model driven by time-dependent electric fields
P. Vemareddy
Aiming to capture the formation and eruption of flux ropes (FRs) in the source active regions (ARs), we simulate the coronal magnetic field evolution of the AR 11429 employing the…