Results 11 to 20 of about 1,069,804 (194)
Solar Filament Eruptions in H α Doppler Velocity [PDF]
The Astrophysical Journal, 2023 We use observations taken with a novel solar telescope spectroheliograph to investigate the association between the early filament rise and coronal mass ejections (CMEs).
I. A. Berezin +2 more
doaj +4 more sources
Falling Threads during Solar Filament Eruptions
The Astrophysical JournalMass drainage is frequently observed in solar filaments. During filament eruptions, falling material most likely flows along magnetic field lines, which may provide important clues for the magnetic structures of filaments.
Yidian Wu +3 more
doaj +4 more sources
SYMPATHETIC SOLAR FILAMENT ERUPTIONS [PDF]
Astrophysical Journal Letters, 2016 ABSTRACT The 2015 March 15 coronal mass ejection as one of the two that together drove the largest geomagnetic storm of solar cycle 24 so far was associated with sympathetic filament eruptions. We investigate the relations between the different filaments involved in the eruption.
Rui Wang, Ivan Zimovets, Huidong Hu
exaly +4 more sources
Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament
The Astrophysical JournalFilament eruptions are magnetically driven violent explosions commonly observed on the Sun and late-type stars, sometimes leading to monster coronal mass ejections that directly affect the nearby planets’ environments.
Hechao Chen +10 more
doaj +2 more sources
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 +4 more sources
Predicting Solar Filament Eruptions With Hek Filament Metadata
, 2015 Solar filaments are cool, dark channels of partially-ionized plasma that lie above the chromosphere. Their structure follows the neutral line between local regions of opposite magnetic polarity. Previous research (e.g. Schmieder et al. 2013) has shown a positive correlation (80%) between the occurrence of filament eruptions and coronal mass ejections ...
Aggarwal, Ashna +1 more
openaire +3 more sources
Filament eruptions and the impulsive phase of solar flares
Astrophysical Journal, 1988 Filament motion during the onset of the solar flare impulsive phase is examined. The impulsive phase onset is established from profiles of about 30 keV X-ray fluxes and the rapid flare brightenings characteristic of the H-alpha flash phase. The filament motion begins several minutes before the impulsive or flash phase of the flare.
S R Kane, S W Kähler, H Zirin
exaly +2 more sources
Two Cases of Non-Radial Filament Eruption and Associated CME Deflection
UniverseThe purpose of this paper is to analyze the multi-wavelength and multi-instrument observations of two quiescent filament eruptions as well as the deflection of associated CMEs from the radial direction.
Kostadinka Koleva +4 more
doaj +2 more sources
Solar filament eruptions and energetic particle events
Astrophysical Journal, 1986 The 1981 December 5 solar filament eruption that is associated with an energetic (E greater than 50 MeV) particle event observed at 1 AU. The eruption was photographed in H-alpha and was observed by the Solwind whitelight coronagraph on P78-1. It occurred well away from any solar active region and was not associated with an impulsive microwave burst ...
N r jr Sheeley, R G Stone, E W Cliver
exaly +2 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