NASA NTRS · 20120004175
Filament Eruption Onset
Abstract
We have been investigating filament eruptions in recent years. Use filament eruptions as markers of the coronal field evolution. Data from SoHO, Yohkoh, TRACE, Hinode, and other sources. We and others have observed: (1)Filaments often show slow rise, followed by fast rise, (2) Brightenings, preflares, microflares during slow rise (3) Magnetic evolution in hours prior to eruption onset. We investigated What do Hinode and SDO show for filament eruptions?
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Sterling, Alphonse C., Moore, Ronald L.. 2011-12-13. Filament Eruption Onset. https://ntrs.nasa.gov/citations/20120004175
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