Small-scale filament eruptions as the driver of X-ray jets in solar coronal holes

Alphonse C. Sterling (), Ronald L. Moore (), David A. Falconer and Mitzi Adams
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Alphonse C. Sterling: NASA/Marshall Space Flight Center
Ronald L. Moore: NASA/Marshall Space Flight Center
David A. Falconer: NASA/Marshall Space Flight Center
Mitzi Adams: NASA/Marshall Space Flight Center

Nature, 2015, vol. 523, issue 7561, 437-440

Abstract: A study of the formation of X-ray jets in solar coronal holes suggests that this process does not follow the popular ‘emerging-flux’ model, but instead results from a minifilament eruption akin to the larger-scale filament eruptions that drive larger solar flares and mass ejections.

Date: 2015
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DOI: 10.1038/nature14556

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