Results 11 to 20 of about 3,305 (196)
Solar filament eruptions and energetic particle events
The 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 ...
S. W. Kahler +5 more
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Solar filament eruptions and their physical role in triggering coronal mass ejections [PDF]
Advances in Space Research, 2013 23 pages, 13 figures ...
Schmieder, B. +2 more
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Filament eruptions and the impulsive phase of solar flares
The 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. W. Kahler +3 more
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SYMPATHETIC SOLAR FILAMENT ERUPTIONS [PDF]
The 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 +5 more
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Sympathetic Partial Filament Eruptions Caused by the Interaction between Two Nearby Filaments
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
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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
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The Astrophysical Journal, 2023 Partial filament eruptions have often been observed; however, the physical mechanisms that lead to filament splitting are not yet fully understood.
Zheng Sun +7 more
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Pre-eruption Splitting of the Double-decker Structure in a Solar Filament [PDF]
The Astrophysical Journal, 2021 Abstract Solar filaments often erupt partially. Although how they split remains elusive, the splitting process has the potential of revealing the filament structure and eruption mechanism. Here we investigate the pre-eruption splitting of an apparently single filament and its subsequent partial eruption on 2012 September 27.
Hanya Pan +6 more
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A comparison study of a solar active-region eruptive filament and a neighboring non-eruptive filament [PDF]
Research in Astronomy and Astrophysics, 2016 Solar active region (AR) 11283 is a very magnetically complex region and it has produced many eruptions. However, there exists a non-eruptive filament in the plage region just next to an eruptive one in the AR, which gives us an opportunity to perform a comparison analysis of these two filaments. The coronal magnetic field extrapolated using a CESE-MHD-
Jiang, Chaowei +3 more
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ACCELERATION PHASES OF A SOLAR FILAMENT DURING ITS ERUPTION [PDF]
The Astrophysical Journal, 2015 11 pages, 3 figures (Accepted by the Astrophysical Journal Letters)
Song, Hongqiang +5 more
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