Three-dimensional Velocity Fields of the Solar Filament Eruptions Detected by CHASE
The eruption of solar filaments, also known as prominences appearing off limb, is a common phenomenon in the solar atmosphere. It ejects massive plasma and high-energy particles into interplanetary space, disturbing the solar-terrestrial environment.
Ye Qiu +5 more
doaj +5 more sources
Why torus-unstable solar filaments experience failed eruption? [PDF]
To investigate the factors that control the success and/or failure of solar eruptions, we study the magnetic field and 3-Dimensional (3D) configuration of 16 filament eruptions during 2010 July - 2013 February.
Cheng, Xin +7 more
core +6 more sources
Solar Filament Eruptions in H α Doppler Velocity
We use observations taken with a novel solar telescope spectroheliograph to investigate the association between the early filament rise and coronal mass ejections (CMEs).
I. A. Berezin +2 more
doaj +2 more sources
Falling Threads during Solar Filament Eruptions
Mass drainage is frequently observed in solar filaments. During filament eruptions, falling material most likely flows along magnetic field lines, which may provide important clues for the magnetic structures of filaments.
Yidian Wu +3 more
doaj +3 more sources
Sympathetic Partial and Full Filament Eruptions Observed in One Solar Breakout Event [PDF]
We report two sympathetic solar eruptions, including a partial and a full flux rope eruption in a quadrupolar magnetic region, where a large and a small filament resided above the middle and the east neutral lines respectively.
Liu, Yu, Shen, Yuandeng, Su, Jiangtao
core +2 more sources
How Reconnection-unfavored Magnetic Flux Emergence Suppresses Solar Filament Eruptions
Magnetic flux emergence is traditionally considered to be a key trigger of solar filament eruptions, yet its role in suppressing filament eruptions remains less understood.
Chengrui Zhou +6 more
doaj +3 more sources
Observations of a Failed Solar Filament Eruption Involving External Reconnection
We report a failed solar filament eruption that involves external magnetic reconnection in a quadrupolar magnetic configuration. The evolution exhibits three phases of kinematic evolution: a slow rise, an acceleration, and a deceleration.
Yuehong Chen +4 more
doaj +3 more sources
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 evidence for the configuration of the pre-eruption filament ...
Yijun Hou +15 more
doaj +3 more sources
Sympathetic Eruption of Two Filaments and Associated Solar Coronal Jet
Combining the high-quality observations from the Solar Dynamics Observatory, the Global Oscillation Network Group, and the Chinese H α Solar Explorer, we report a solar coronal jet triggered by the sympathetic eruption of two filaments on 2024 January 11.
Jiayan Yang +6 more
doaj +3 more sources
Reconnection Nanojets in an Erupting Solar Filament with Unprecedented High Speeds
Solar nanojets are small-scale jets generated by component magnetic reconnection, characterized by collimated plasma motion perpendicular to the reconnecting magnetic field lines.
Yuhang Gao +6 more
doaj +4 more sources

