activity
20092026
most citedThe FIP and Inverse FIP Effects in Solar and Stellar Coronae

334 citations · 703 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2026

Ejecta clumps revealed by study of reverse-shocked ejecta through MUSE integral field spectroscopy of SNR 0509-67.5

Priyam Das, Ivo Seitenzahl, J. Martin Laming +3

We report the discovery of a spatially resolved clumpy ejecta structure in the reverse-shocked ejecta of SNR 0509-67.5, revealed through multiple faint and broad forbidden coronal…

astro-ph.SR2026★ 2 cited

Helium emission from Balmer-dominated shocks in Type Ia supernova remnants provides constraints to their progenitor systems

Priyam Das, Ivo Rolf Seitenzahl, Parviz Ghavamian +4

Balmer-dominated shocks in Type Ia supernova remnants offer powerful probes into collisionless shock physics and hints towards supernova progenitor environments. Prior studies focu…

astro-ph.SR2026

Chromospheric dynamics and turbulence regulate the solar FIP effect

Andy S. H. To, J. Martin Laming, Jeffrey Reep +1

Elemental abundance variations in the solar corona, commonly characterised by First Ionisation Potential (FIP) bias, provide crucial diagnostics of chromospheric processes. The pon…

astro-ph.SR2025★ 1 cited

Radiative hydrodynamic simulations of FIP fractionation in solar flares

Jeffrey W. Reep, Luke Fushimi Benavitz, Andy S. H. To +5

Elemental abundances in solar flares are observed to vary both spatially and temporally, but the underlying mechanisms remain poorly understood. There is an interplay between advec…

astro-ph.SR2025

FIP Bias Evolution in an Emerging Active Region as observed in SPICE Synoptic Observations

T. Varesano, D. M. Hassler, N. Zambrana Prado +6

We investigate the time evolution of relative elemental abundances in the context of the first ionization potential effect focusing on an active region. Our aim is to characterize…

astro-ph.SR2024

Searching for evidence of subchromospheric magnetic reconnection on the Sun

D. Baker, L. van Driel-Gesztelyi, A. W. James +13

Within the coronae of stars, abundances of those elements with low first ionization potential (FIP) often differ from their photospheric values. The coronae of the Sun and solar-ty…