5 citations · 5 across the 2 of their papers we have counts for
2 papers
astro-ph.SR2025
Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
Julien Poyatos, Octavi Fors, José Maria Gómez Cama
Stellar flares are intense bursts of radiation caused by magnetic reconnection on active stars. They are especially frequent on M dwarfs, where they can significantly influence the…
astro-ph.SR2023★ 5 cited
Coronal voids and their magnetic nature
J. D. Nölke, S. K. Solanki, J. Hirzberger +68
Extreme ultraviolet (EUV) observations of the quiet solar atmosphere reveal extended regions of weak emission compared to the ambient quiescent corona. The magnetic nature of these…