most citedTemporal Variation of Flare Occurrence Rates via the Spot Evolution on the Sun and Solar-type Stars

3 citations · 4 across the 3 of their papers we have counts for

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astro-ph.SR2026

Magnetic Heating Across the Sun and Solar-like Stars: Universal Scaling Laws from Chromospheres to Coronae

Shin Toriumi, Kosuke Namekata, Yuta Notsu +2

Magnetic activity in cool stars governs the thermal structure and high-energy radiative output of their outer atmospheres, thereby influencing stellar evolution, stellar winds, and…

astro-ph.SR2026

A systematic study of quiescent and outburst properties of X-ray-bright young stellar objects using XMM-Newton

Koki Sakuta, Ikuyuki Mitsuishi, Seiya Sasamata +6

Young Stellar Objects (YSOs) exhibit strong X-ray emission, widely attributed to magnetic reconnection and magnetospheric accretion; however, owing primarily to limited photon stat…

astro-ph.SR2026★ 1 cited

Pre-flare and active region plasma flows and structure seen by the short wavelength camera on SOLAR-C/EUVST

James McKevitt, Sarah Matthews, David H. Brooks +20

The mechanisms triggering solar flares and driving coronal heating occur across wide temperature ranges on small spatial scales and short timescales, making them difficult to obser…

astro-ph.SR2025

Origin of the stellar Fe Kα line clarified with FUV and X-ray observations of a superflare on the RS Canum Venaticorum-type Star UX Arietis

Shun Inoue, Wataru Buz Iwakiri, Tomoki Kimura +11

Fluorescence line diagnostics of the Fe Kα line at keV observed in both solar and stellar flares can constrain the latitude and size of the flare loop, even in the absen…

astro-ph.SR2025★ 3 cited

Temporal Variation of Flare Occurrence Rates via the Spot Evolution on the Sun and Solar-type Stars

Takato Tokuno, Kosuke Namekata, Hiroyuki Maehara +1

The spot evolution on the Sun and solar-type stars is important for understanding the nature of consequential flaring activity. This study statistically investigates the variance o…