Results 121 to 130 of about 549 (204)
Miniature Filament Eruptions and their Reconnections in X-Ray Jets: Evidence for a New Paradigm [PDF]
We investigate the onset of approximately10 random X-ray jets observed by Hinode/XRT. Each jet was near the limb in a polar coronal hole, and showed a ``bright point'' in an edge of the base of the jet, as is typical for previously-observed X-ray jets ...
Sterling, Alphonse C. +2 more
core +1 more source
Failed filament eruptions have been reported previously; however, the responsible physical mechanisms remain debated. Using multiwavelength data from Solar Orbiter and Solar Dynamics Observatory, we analyze a failed filament eruption on 2024 March 19 ...
Yue Fang +5 more
doaj +1 more source
Flares are intense explosions on the solar and stellar surfaces, and solar flares are sometimes accompanied by filament or prominence eruptions. Recently, a large filament eruption associated with a superflare on a solar-type star EK Dra was discovered ...
Kai Ikuta, Kazunari Shibata
doaj +1 more source
Ultra-high-resolution observations of persistent null-point reconnection in the solar corona. [PDF]
Cheng X +23 more
europepmc +1 more source
Although multiscale filament eruptions serve as significant triggers for various energetic release processes in the solar atmosphere, the underlying mechanisms remain elusive.
Liping Yang +13 more
doaj +1 more source
Initiation of Solar Eruptions: Recent Observations and Implications for Theories [PDF]
Solar eruptions involve the violent disruption of a system of magnetic field. Just how the field is destabilized and explodes to produce flares and coronal mass ejections (CMEs) is still being debated in the solar community.
Sterling, A. C.
core
The southward component of the interplanetary magnetic field, often originating from solar coronal mass ejections (CMEs), plays a crucial role in driving geomagnetic storms. Accurate prediction of the flux rope orientation of CMEs as they arrive at Earth
Ying Wang +6 more
doaj +1 more source
Automated High-Precision Recognition of Solar Filaments Based on an Improved U2-Net
Solar filaments are a significant solar activity phenomenon, typically observed in full-disk solar observations in the H-alpha band. They are closely associated with the magnetic fields of solar active regions, solar flare eruptions, and coronal mass ...
Wendong Jiang, Zhengyang Li
doaj +1 more source
Diverse glasses revealed from Chang'E-5 lunar regolith. [PDF]
Zhao R +15 more
europepmc +1 more source
Dynamics of An Erupting Filament and a Coronal Loop during Their Interaction
Although interactions between filaments and other atmospheric structures are frequently observed, detailed studies on how these interactions affect the dynamics of the involved structures remain scarce.
Yue Fang +3 more
doaj +1 more source

