Sun-as-a-star Observations of Obscuration Dimmings Caused by Filament Eruptions [PDF]
The Astrophysical JournalFilament eruptions often lead to coronal mass ejections (CMEs) on the Sun and are one of the most energetic eruptive phenomena in the atmospheres of other late-type stars.
Yu Xu +3 more
doaj +5 more sources
Solar filament eruptions and their physical role in triggering coronal mass ejections [PDF]
Advances in Space Research, 2013 23 pages, 13 figures ...
Guillaume Aulanier +2 more
exaly +4 more sources
Why Do Torus-unstable Solar Filaments Experience Failed Eruptions? [PDF]
The Astrophysical Journal Letters, 2019 Abstract We study the magnetic field and 3D configuration of 16 filament eruptions during 2010 July–2013 February in order to investigate the factors that control the success and/or failure of solar eruptions. All of these events, i.e., eruptions that failed to be ejected and become coronal mass ejections, have filament maximum heights ...
Zhenjun 振军 Zhou 周 +7 more
openaire +6 more sources
Prediction of Solar Eruptions Using Filament Metadata
Astrophysical Journal, Supplement Series, 2018 Abstract We perform a statistical analysis of erupting and non-erupting solar filaments to determine the properties related to the eruption potential. In order to perform this study, we correlate filament eruptions documented in the Heliophysics Event Knowledgebase (HEK) with HEK filaments that have been grouped together using a ...
Rafal Angryk +2 more
exaly +2 more sources
Quantification of the Writhe Number of the Evolution of Solar Filament Axes [PDF]
The Astrophysical Journal, 2023 Solar filament eruptions often show complex and dramatic geometric deformation that is highly relevant to the underlying physical mechanism triggering the eruptions.
Zhenjun Zhou +5 more
doaj +2 more sources
Observations of a Failed Solar Filament Eruption Involving External Reconnection
The Astrophysical Journal, 2023 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
The Astrophysical Journal, 2023 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
Observational Evidence of the Kink Instability in Solar Filament Eruptions and Sigmoids [PDF]
Astrophysical Journal, 2005 Two lines of observational evidence are used to infer that the MHD helical kink instability is associated with solar eruptions. The senses of twist and writhe are determined in images of seven erupting filaments obtained at 10830, 1600, 195, and 171 ?. In every case the sense of twist is the same as the sense of writhe, as required for a kink.
D M Rust, B J Labonte
exaly +2 more sources
Three-dimensional Velocity Fields of the Solar Filament Eruptions Detected by CHASE
The Astrophysical Journal LettersThe 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 +3 more sources
Sympathetic Eruption of Two Filaments and Associated Solar Coronal Jet
The Astrophysical JournalCombining 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