Results 11 to 20 of about 549 (204)
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 +6 more sources
Observing the release of twist by magnetic reconnection in a solar filament eruption. [PDF]
Nat Commun, 2016 AbstractMagnetic reconnection is a fundamental process of topology change and energy release, taking place in plasmas on the Sun, in space, in astrophysical objects and in the laboratory. However, observational evidence has been relatively rare and typically only partial.
Xue Z +11 more
europepmc +8 more sources
Sympathetic Partial Filament Eruptions Caused by the Interaction between Two Nearby Filaments [PDF]
The Astrophysical Journal, 2023 To better understand the physical connections in sympathetic solar eruptions, we investigated the interaction between two nearby filaments and their successive partial eruptions in the active region (AR) NOAA 12866 on 2021 September 9 by using data from ...
Liping Yang +9 more
doaj +2 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 [PDF]
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
Heating of Quiescent Coronal Loops Caused by Nearby Eruptions Observed with the Solar Dynamics Observatory and the Solar Upper Transition Region Imager [PDF]
The Astrophysical Journal, 2023 How structures, e.g., magnetic loops, in the upper atmosphere, i.e., the transition region and corona, are heated and sustained is one of the major unresolved issues in solar and stellar physics.
Leping Li +7 more
doaj +3 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 +3 more sources
Two Cases of Non-Radial Filament Eruption and Associated CME Deflection [PDF]
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
Predicting Solar Filament Eruptions With Hek Filament Metadata [PDF]
, 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
The role of filament activation in a solar eruption [PDF]
Astronomy & Astrophysics, 2012 Observations show that the mutual relationship between filament eruptions and solar flares cannot be described in terms of an unique scenario. In some cases, the eruption of a filament appears to trigger a flare, while in others the observations are more consistent with magnetic reconnection that produces both the flare observational signatures (e.g ...
da Costa F. Rubio +4 more
openaire +5 more sources