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Yuta Notsu

University of Colorado System
H指数:19
被引数:1,903

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Origin of the Stellar Fe Kα Line Clarified with Far-ultraviolet and X-Ray Observations of a Superflare on the RS Canum Venaticorum-type Star UX Arietis

通过RS Canum Venaticorum型恒星UX Arietis的超耀斑的远紫外和X射线观测澄清恒星Fe Kα线的起源

2026-05-010
PRE
Multiwavelength Campaign Observations of a Young Solar-type Star; EK Draconis. III. Comparison between Starspot Mapping; Zeeman Doppler Imaging; and Multiwavelength Variability

多波长观测活动对年轻太阳型恒星EK Draconis的研究;III. 恒星黑子成像、塞曼多普勒成像与多波长变异性之间的比较

2026-04-020
OAAI
High-time-cadence Spectroscopy and Photometry of Stellar Flares on M-dwarf YZ Canis Minoris with Seimei Telescope and TESS. II. Statistical Properties of Blue/Red Asymmetries in the Hα Line

高时间分辨率的 M-dwarf YZ Canis Minoris 恒星耀斑的光谱和测光研究,以及 Seimei 望远镜和 TESS 数据。II. Hα 线中蓝/红不对称性的统计特性

2025-05-200
OA
Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-driven Modeling and Observed Magnetic Environment
2024-11-270
OA
Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data
2024-01-2514
OA
Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares
2024-01-1117
OA
Extreme Solar Events: Setting up a Paradigm

极端太阳事件: 建立一个范式

2023-11-0311
OA