3 papers
astro-ph.SR2026
Chromospheric magnetic field extrapolations reveal the flux-rope configuration of a solar filament
Robert Jarolim, João M. da Silva Santos, Matthias Rempel +5
Solar eruptions are powered by the release of magnetic energy stored in the lower solar atmosphere, but the pre-eruptive magnetic configuration of filament channels remains difficu…
astro-ph.SR2025
Understanding the magnetic field and plasma- along umbral fan loops traced using 3-min slow waves
Ananya Rawat, Girjesh Gupta, Tom Van Doorsselaere +2
The plasma- is an important fundamental physical quantity in solar plasma physics, which determines the dominating process in the solar atmosphere, i.e., magnetic or thermodyna…
astro-ph.SR2025
The Relation between Solar Spicules and Magnetohydrodynamic Shocks
Sankalp Srivastava, Piyali Chatterjee, Sahel Dey +1
Spicules are thin, elongated jet-like features seen in observations of the solar atmosphere, at the interface between the solar photosphere and the corona. These features exhibit h…