Theory of coronal X-ray jets

Details Theory of coronal X-ray jets Theory of coronal X-ray jets

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471...61y&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 61-66 (1999).

Physics

1

Scientific paper

We review our magnetic reconnection model of the solar coronal X-ray jets. The plasma of an X-ray jet is accelerated and heated by reconnection between the emerging flux and a pre-existing coronal field. Many observed characteristics of the X-ray jets could be successfully reproduced through the two-dimensional MHD numerical simulations based on this model. We also discuss the Alfvén wave generated by the reconnection process. The simulation results show that the amount of Alfvén wave energy is ~3% of the total energy released by the magnetic reconnection.

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