Coronal X-ray jets

Details Coronal X-ray jets Coronal X-ray jets

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382...18s&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 18-

Physics

2

Particle Emission, Solar Wind

Scientific paper

The soft X-ray telescope (SXT) aboard Yohkoh has discovered coronal X-ray jets associated with small flares (microflares-subflares) in X-ray bright points (XBPs), emerging flux regions (EFRs), or active regions (ARs). These newly discovered jets may provide clues to solving the coronal heating mechanism and acceleration of high speed solar wind. The recent development of observations and theoretical modeling of X-ray jets are reviewed with emphasis upon the role of magnetic reconnection in generating these jets.

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