Classification of magnetic reconnection during two current-loop coalescence

Details Classification of magnetic reconnection during two current-loop coalescence Classification of magnetic reconnection during two current-loop coalescence

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..142..399s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 142, no. 2, p. 399-402.

Physics

20

Coronal Loops, Magnetic Field Reconnection, Solar Activity Effects, Solar Corona, Solar Flares, Solar Magnetic Field, Coalescing, Solar Maximum Mission, X Ray Telescopes

Scientific paper

We present a classification of magnetic reconnection during two current loop coalescence, which may be quite important for the physical process of both solar flares and coronal loop heating in the solar active region. It is suggested that different kinds of the current loop coalescence processes could be identified from the soft X-ray telescope of the 'Yohkoh' satellite and the magnetic field data in the active region.

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