Various Features of the X-class White-light Flares in Super Active Region NOAA 13664
Y Li, X Liu, Z Jing, W Chen, Q Li, Y Su… - The Astrophysical …, 2024 - iopscience.iop.org
Super active region NOAA 13664 produced 12 X-class flares (including the largest one so
far, an occulted X8. 7 flare, in solar cycle 25) during 2024 May 8–15, and 11 of them are …
far, an occulted X8. 7 flare, in solar cycle 25) during 2024 May 8–15, and 11 of them are …
The near-ultraviolet continuum radiation in the impulsive phase of HF/GF-type dMe flares. I. Data
AF Kowalski, JP Wisniewski, SL Hawley… - The Astrophysical …, 2019 - iopscience.iop.org
We present near-UV (NUV) flare spectra from the Hubble Space Telescope (HST)/Cosmic
Origins Spectrograph during two moderate-amplitude U-band flares on the dM4e star GJ …
Origins Spectrograph during two moderate-amplitude U-band flares on the dM4e star GJ …
A statistical study of solar white-light flares observed by the white-light solar telescope of the Lyman-alpha solar telescope on the Advanced Space-based Solar …
Z Jing, Y Li, L Feng, H Li, Y Huang, Y Li, Y Su, W Chen… - Solar Physics, 2024 - Springer
Solar white-light flares (WLFs) are those accompanied by brightenings in the optical
continuum or integrated light. The White-light Solar Telescope (WST), as an instrument of …
continuum or integrated light. The White-light Solar Telescope (WST), as an instrument of …
Circular-ribbon flares and the related activities
Q Zhang - Reviews of Modern Plasma Physics, 2024 - Springer
Solar flares are an impulsive increase of emissions as a result of impetuous release of
magnetic free energy. This paper will present the recent progress on circular-ribbon flares …
magnetic free energy. This paper will present the recent progress on circular-ribbon flares …
The Lyman-alpha Solar Telescope (LST) for the ASO-S mission—I. Scientific objectives and overview
H Li, B Chen, L Feng, Y Li, Y Huang… - … in Astronomy and …, 2019 - iopscience.iop.org
As one of the payloads for the Advanced Space-based Solar Observatory (ASO-S) mission,
the Lyman-alpha (Lyα) Solar Telescope (LST) is aimed at imaging the Sun and the inner …
the Lyman-alpha (Lyα) Solar Telescope (LST) is aimed at imaging the Sun and the inner …
A Possible Mechanism for the “Late Phase” in Stellar White-light Flares
M dwarf flares observed by the Transiting Exoplanet Survey Satellite (TESS) sometimes
exhibit a peak-bump light-curve morphology, characterized by a secondary, gradual peak …
exhibit a peak-bump light-curve morphology, characterized by a secondary, gradual peak …
Detections of multi-periodic oscillations during a circular ribbon flare
Z Ning, Y Wang, Z Hong, D Li - Solar Physics, 2022 - Springer
We present the analysis of three kinds of oscillating behavior using multi-wavelength
observations of the 10 November 2013 (SOL2013-11-10T05: 14) circular-ribbon flare. This …
observations of the 10 November 2013 (SOL2013-11-10T05: 14) circular-ribbon flare. This …
Space weather related to solar eruptions with the ASO-S mission
The Advanced Space-based Solar Observatory (ASO-S) is a mission aiming at exploring
solar flares, coronal mass ejections (CMEs), solar magnetic field and their relationships. To …
solar flares, coronal mass ejections (CMEs), solar magnetic field and their relationships. To …
EXTraS discovery of an X-ray superflare from an L dwarf
A De Luca, B Stelzer, AJ Burgasser… - Astronomy & …, 2020 - aanda.org
We present the first detection of an X-ray flare from an ultracool dwarf of spectral class L. The
event was identified in the EXTraS database of XMM-Newton variable sources, and its …
event was identified in the EXTraS database of XMM-Newton variable sources, and its …
[HTML][HTML] 空间太阳物理学科发展战略研究
颜毅华， 邓元勇， 甘为群， 丁明德， 田晖， 朱小帅 - 空间科学学报, 2023 - cjss.ac.cn
太阳物理学是研究太阳上发生的物理过程及其对行星际空间环境影响的学科.
太阳是人类唯一可以进行细致探测的恒星, 也是天然的多尺度过程并存的等离子体实验室, 同时 …
太阳是人类唯一可以进行细致探测的恒星, 也是天然的多尺度过程并存的等离子体实验室, 同时 …