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Long-term evolution of decayless kink oscillations of solar coronal loops
Monthly notices of the Royal Astronomical Society, 2022 Long-term evolution of instantaneous parameters of decayless kink oscillations of six solar coronal loops observed for longer than two hours each, is studied.
S. Zhong +3 more
semanticscholar +1 more source
Non-thermal line broadening due to braiding-induced turbulence in solar coronal loops [PDF]
Astronomy & Astrophysics, 2020 Aims. Emission line profiles from solar coronal loops exhibit properties that are unexplained by current models. We investigate the non-thermal broadening associated with plasma heating in coronal loops that is induced by magnetic field line braiding ...
D. Pontin, H. Peter, L. P. Chitta
semanticscholar +1 more source
Traveling kink oscillations of coronal loops launched by a solar flare [PDF]
Astronomy & Astrophysics, 2023 We investigate the traveling kink oscillation triggered by a solar flare on 2022 September 29. The observational data is mainly measured by the Solar Upper Transition Region Imager (SUTRI), the Atmospheric Imaging Assembly (AIA), and the Spectrometer ...
Dong Li +7 more
semanticscholar +1 more source
Coronal Loop Detection Using Multiscale Convolutional Neural Networks
The Astrophysical Journal Supplement Series, 2023 Solar magnetic fields play an important role in many solar activities, such as the solar wind, coronal mass ejections, and coronal oscillation. Coronal loops are curvilinear structures in the solar atmosphere and are closely related to coronal magnetic ...
Yunzhi Wang, Bo Liang, Song Feng
doaj +1 more source
The Astrophysical Journal, 2023 We present the observations of multimode kink waves and a narrow quasiperiodic fast-propagating (QFP) wave train in association with a jet on 2011 December 11.
Zhining Qu +5 more
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Formation of Solar Quiescent Coronal Loops through Magnetic Reconnection in an Emerging Active Region [PDF]
Astrophysical Journal, 2021 Coronal loops are the building blocks of solar active regions. However, their formation mechanism remains poorly understood. Here we present direct observational evidence for the formation of coronal loops through magnetic reconnection as new magnetic ...
Zhenyong Hou +8 more
semanticscholar +1 more source
Quasi-periodic Fast Propagating Magnetoacoustic Waves during the Magnetic Reconnection Between Solar Coronal Loops [PDF]
Astrophysical Journal, 2018 Employing Solar Dynamics Observatory/Atmospheric Imaging Assembly (AIA) multi-wavelength images, we have presented coronal condensations caused by magnetic reconnection between a system of open and closed solar coronal loops.
Leping Li +7 more
semanticscholar +1 more source
Helical Twisting Number and Braiding Linkage Number of Solar Coronal Loops [PDF]
Astrophysical Journal, 2019 Coronal loops in active regions are often characterized by quasi-circular and helically twisted (sigmoidal) geometries, which are consistent with dipolar potential field (PF) models in the former case, and with nonlinear force-free field models with ...
M. Aschwanden
semanticscholar +1 more source
A Possible Mechanism for the “Late Phase” in Stellar White-light Flares
The Astrophysical Journal, 2023 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 well after the main, impulsive peak.
Kai E. Yang +3 more
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The Astrophysical Journal, 2023 The EUI instrument on the Solar Orbiter spacecraft has obtained the most stable, high-resolution images of the solar corona from its orbit with a perihelion near 0.4 au.
P. G. Judge
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