Coronal X-ray Jets

Details Coronal X-ray Jets Coronal X-ray Jets

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp...75s&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.75-78.

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Scientific paper

The soft X-ray telescope (SXT) aboard Yohkoh has discovered coronal X-ray jets associated with small flares in XBPs, EFRs, or ARs. The common observed characteristics of these jets are discussed mainly from morphological points of view. It is suggested that magnetic reconnection between emerging magnetic flux and the overlying coronal/chromospheric magnetic field is a key physical process for producing these jets.

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