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- Title
Small-scale filament eruptions as the driver of X-ray jets in solar coronal holes.
- Authors
Sterling, Alphonse C.; Moore, Ronald L.; Falconer, David A.; Adams, Mitzi
- Abstract
Solar X-ray jets are thought to be made by a burst of reconnection of closed magnetic field at the base of a jet with ambient open field. In the accepted version of the 'emerging-flux' model, such a reconnection occurs at a plasma current sheet between the open field and the emerging closed field, and also forms a localized X-ray brightening that is usually observed at the edge of the jet's base. Here we report high-resolution X-ray and extreme-ultraviolet observations of 20 randomly selected X-ray jets that form in coronal holes at the Sun's poles. In each jet, contrary to the emerging-flux model, a miniature version of the filament eruptions that initiate coronal mass ejections drives the jet-producing reconnection. The X-ray bright point occurs by reconnection of the 'legs' of the minifilament-carrying erupting closed field, analogous to the formation of solar flares in larger-scale eruptions. Previous observations have found that some jets are driven by base-field eruptions, but only one such study, of only one jet, provisionally questioned the emerging-flux model. Our observations support the view that solar filament eruptions are formed by a fundamental explosive magnetic process that occurs on a vast range of scales, from the biggest mass ejections and flare eruptions down to X-ray jets, and perhaps even down to smaller jets that may power coronal heating. A similar scenario has previously been suggested, but was inferred from different observations and based on a different origin of the erupting minifilament.
- Subjects
CORONAL holes; CORONAL mass ejections; SOLAR x-rays; X-ray bursts; X-ray astronomy; SOLAR activity; SOLAR filaments
- Publication
Nature, 2015, Vol 523, Issue 7561, p437
- ISSN
0028-0836
- Publication type
Article
- DOI
10.1038/nature14556