Observation and modelling of solar jets. [PDF]
Shen Y.
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
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
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
Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections. [PDF]
Nitta NV +16 more
europepmc +1 more source
Chromospheric Magnetic Field Extrapolations Reveal the Flux-rope Configuration of a Solar Filament
Solar eruptions are powered by the release of magnetic energy stored in the lower solar atmosphere, but the preeruptive magnetic configuration of filament channels remains difficult to determine.
Robert Jarolim +7 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
Filament Eruptions, Jets, and Space Weather [PDF]
Previously, from chromospheric H alpha and coronal Xray movies of the Sun's polar coronal holes, it was found that nearly all coronal jets (greater than 90%) are one or the other of two roughly equally common different kinds, different in how they erupt:
Cirtain, Jonathan +4 more
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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
Observation of sulphate aerosols and SO2 from volcanic eruptions using data from the Atmospheric Chemistry Experiment (ACE) [PDF]
Infrared spectra measured by the Atmospheric Chemistry Experiment Fourier Transform Spectrometer (ACE-FTS) on board of the SCISAT satellite were used to analyse the temporal and spatial evolution of volcanic aerosols from the Kasatochi (August 2008 ...
Doeringer, Debora
core

