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20142026
most citedModeling a Carrington-scale Stellar Superflare and Coronal Mass Ejection from

37 citations · 50 across the 16 of their papers we have counts for

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astro-ph.SR2025

X-ray Evolution of Young Stars: Early Dimming and Coronal Softening in Solar-Mass Stars with Implications for Planetary Atmospheres

Konstantin V. Getman, Eric D. Feigelson, Vladimir S. Airapetian +1

X-ray and ultraviolet (XUV) emission from young stars plays a critical role in shaping the evolution of planetary atmospheres and the conditions for habitability. To assess the lon…

astro-ph.SR2025★ 6 cited

Discovery of multi-temperature coronal mass ejection signatures from a young solar analogue

Kosuke Namekata, Kevin France, Jongchul Chae +14

Coronal mass ejections (CMEs) on the early Sun may have profoundly influenced the planetary atmospheres of early Solar System planets. Flaring young solar analogues serve as excell…

astro-ph.EP2025

Extreme Geomagnetic Storm on Early Earth Induced by Corotating Interaction Regions from the Young Sun

Dibyendu Sur, Vladimir S. Airapetian

Recent multiwavelength observations of young solar analogs suggest that the young Sun in the first 600 Myr was a magnetically active star that produced an X-ray and Extreme-UV (EUV…

astro-ph.SR2025

Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M dwarf

Atul Mohan, Peter H. Hauschildt, Birgit Fuhrmeister +3

Millimeter (mm) emission from F - M dwarfs (cool stars) primarily traces chromospheric activity, with thermal emission thought to dominate in quiescence. Despite the high chromosph…

astro-ph.SR2025

A Semi-Empirical Estimate of Solar EUV Evolution from 10 Myr to 10 Gyr

Kevin France, Girish Duvvuri, Cynthia Froning +9

The extreme-ultraviolet (EUV; 100 -- 911 Å) spectra of F, G, K, and M stars provide diagnostics of the stellar chromosphere through the corona, with line and continuum formation te…

astro-ph.SR2025

Multi-Observatory Study of Young Stellar Energetic Flares (MORYSEF): No Evidence For Abnormally Strong Stellar Magnetic Fields After Powerful X-ray Flares

Konstantin V. Getman, Oleg Kochukhov, Joe P. Ninan +9

We explore the empirical power-law relationship between X-ray luminosity (Lx) and total surface magnetic flux (Phi), established across solar magnetic elements, time- and disk-aver…