Partial Eruption of Solar Filaments. I. Configuration and Formation of Double-decker Filaments
Partial eruptions of solar filaments are the typical representatives of solar eruptive behavior
diversity. Here we investigate a typical filament partial eruption event and present integrated …
diversity. Here we investigate a typical filament partial eruption event and present integrated …
Modelling the magnetic structure of a large-scale horse-shoe-like filament in a decaying and diffuse active region
K Kang, Y Guo, II Roussev… - Monthly Notices of the …, 2023 - academic.oup.com
ABSTRACT A large-scale, horse-shoe-like filament was investigated and the magnetic field
around it was reconstructed. This is an intermediate filament (IF) that appeared on the solar …
around it was reconstructed. This is an intermediate filament (IF) that appeared on the solar …
Negative-energy waves in the vertical threads of a solar prominence
Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination
owing to their threadlike features and dynamic behaviors. Utilizing data from the New …
owing to their threadlike features and dynamic behaviors. Utilizing data from the New …
Formation of a long filament through the connection of two filament segments observed by CHASE
HT Li, X Cheng, YW Ni, C Li, SH Rao… - The Astrophysical …, 2023 - iopscience.iop.org
We present imaging and spectroscopic diagnostics of a long filament during its formation
with the observations from the Chinese Hα Solar Explorer and Solar Dynamics Observatory …
with the observations from the Chinese Hα Solar Explorer and Solar Dynamics Observatory …
Onset mechanism of an inverted U-shaped solar filament eruption revealed by NVST, SDO, and STEREO-A observations
J Wang, X Yan, Q Cai, Z Xue, L Yang, Q Li… - arXiv preprint arXiv …, 2024 - aanda.org
Context. Solar filaments, also called solar prominences when appearing on the solar limb,
consist of dense, cool plasma suspended in the hot and tenuous corona. They are the main …
consist of dense, cool plasma suspended in the hot and tenuous corona. They are the main …
Formation and Evolution of Transient Prominence Bubbles Driven by Erupting Mini-filaments
Y Guo, Y Hou, T Li, Y Shen, J Wang, J Zhang… - arXiv preprint arXiv …, 2024 - arxiv.org
Prominence bubbles, the dark arch-shaped" voids" below quiescent prominences, are
generally believed to be caused by the interaction between the prominences and the slowly …
generally believed to be caused by the interaction between the prominences and the slowly …