Results 91 to 100 of about 1,069,804 (194)
We have studied a B-class solar flare and an associated filament eruption through multiwavelength observations. The flare is triggered at 16:24 UT on 2017 June 7 from Active Region(AR) 12661, and it maximizes at 16:54 UT.
B. Suresh Babu +3 more
doaj +1 more source
Initiation and early kinematic evolution of solar eruptions
We investigate the initiation and early evolution of 12 solar eruptions, including six active-region hot channel and six quiescent filament eruptions, which were well observed by the Solar Dynamics Observatory, as well as by the Solar Terrestrial ...
Török, Tibor +7 more
core +2 more sources
Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel
Similar to the cases of anemone jets, two-sided loop solar jets can also be produced by either flux emergence from the solar interior or small-scale filament eruptions.
Jiayan Yang +4 more
doaj +1 more source
Reconnection Nanojets in an Erupting Solar Filament with Unprecedented High Speeds
Abstract Solar nanojets are small-scale jets generated by component magnetic reconnection, characterized by collimated plasma motion perpendicular to the reconnecting magnetic field lines. As an indicator of nanoflare events, they are believed to play a significant role in coronal heating.
Yuhang Gao +6 more
openaire +4 more sources
Successive filament eruptions within one solar breakout event [PDF]
AbstractThe magnetic breakout model has been widely used to explain solar eruptive activities. Here, we apply it to explain successive filament eruptions occurred in a quadrupolar magnetic source region. Based on the high temporal and spatial resolution, multi-wavelengths observations taken by the Atmospheric Imaging Assembly (AIA) on board the Solar ...
openaire +2 more sources
A Universal Model for Solar Eruptions [PDF]
Magnetically driven eruptions on the Sun, from stellar-scale coronal mass ejections1 to small-scale coronal X-ray and extreme-ultraviolet jets, have frequently been observed to involve the ejection of the highly stressed magnetic flux of a filament ...
Devore, C. Richard +5 more
core +1 more source
Supra-arcade Downflows in an Extensive Fan Associated with a Giant Quiescent Solar Filament Eruption
We investigate the aftermath of a giant quiescent solar filament eruption on 2023 December 24. One feature of the eruption is an extensive fan above the filament channel that is about 3 times as wide as similar structures that appear above active regions
Xiaoyan Xie +8 more
doaj +1 more source
The Noneruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region Emergence
The unpredictability of solar filament eruptions presents major challenges for forecasting space weather, since such eruptions frequently drive coronal mass ejections that impact the heliosphere.
James McKevitt +15 more
doaj +1 more source
On 2024 July 25, while observing the solar active region NOAA 13762 with the high-resolution 1.6 m Goode Solar Telescope at the Big Bear Solar Observatory, we witnessed two mysterious phenomena: the partial detachment of filament strands from its main ...
Ju Jing +8 more
doaj +1 more source
Investigating an Erupting Metric-decimetric Radio Depression and Its Physical Origin
We present direct metric-decimetric radio imaging observations of a fascinating quiescent filament eruption on 2024 March 17 using data from the DAocheng Radio Telescope, with a combination of the Solar Dynamics Observatory and the Chinese H α Solar ...
B. T. Wang +10 more
doaj +1 more source

