Results 1 to 10 of about 549 (204)
Observation and modelling of solar jets. [PDF]
Shen Y.
europepmc +1 more source
Minifilaments are widespread small-scale structures in the solar atmosphere. To better understand their formation and eruption mechanisms, we investigate the entire life of a sigmoidal minifilament located below a large quiescent filament observed by Big
Weilin Teng +8 more
doaj +1 more source
Solar X-ray and EUV imager on board the FY-3E satellite. [PDF]
Chen B +45 more
europepmc +1 more source
Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections. [PDF]
Nitta NV +16 more
europepmc +1 more source
Observational Evidence of Solar Spicules Associated with Microfilament Eruptions Using DKIST
The formation mechanism of spicules is fundamentally important for understanding mass and energy transport from the chromosphere into the corona. Recent studies suggested that spicules may be powered by microfilament eruptions.
Qifan Dong +10 more
doaj +1 more source
Magnetic Structure and Propagation of Two Interacting CMEs From the Sun to Saturn. [PDF]
Palmerio E +16 more
europepmc +1 more source
We study the formation of four coronal mass ejections (CMEs) originating from homologous blowout jets. All of the blowout jets originated from NOAA Active Region (AR) 11515 on 2012 July 2, within a time interval of ≈14 hr.
Binal D. Patel +3 more
doaj +1 more source
Probing Upflowing Regions in the Quiet Sun and Coronal Holes. [PDF]
Schwanitz C +7 more
europepmc +1 more source
Two-stage Primary Acceleration in Filament Initial Eruption under a Fan–Spine Magnetic Configuration
Understanding the filament rising process is crucial for unveiling the triggering mechanisms of coronal mass ejections and forecasting space weather. In this paper, we present a detailed study of the filament initial eruption under a fan–spine structure.
Haitang Li +8 more
doaj +1 more source
Research into the Magnetic Configuration of Eruptive Filaments with a High-class Flare
Filament eruptions are the source of coronal mass ejections, and these phenomena are likely to pose a serious threat to space weather safety. The magnetic structures that carry the filament material are considered the core structures of the eruption, and
Chang Zhang +3 more
doaj +1 more source

