Abstract The resistive MHD equations are numerically solved in two dimensions for an initial-boundary-value problem which simulates reconnection between an emerging magnetic flux region and an overlying coronal magnetic field. The solution involves both ideal-MHD and resistive-MHD processes, and the solution shows an evolution which is remarkably suggestive of the preflare, impulsive, and main phases of the flare-cycle.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    Numerical simulation of reconnection in an emerging magnetic flux region


    Contributors:

    Published in:

    Publication date :

    1984-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English




    Numerical simulation of magnetic reconnection associated with emerging flux in the solar atmosphere

    Yokoyama, T. / Shibata, K. | British Library Online Contents | 1993


    3-D Reconnection Related to New Emerging Flux

    Schmieder, B. / Demoulin, P. / Aulanier, G. et al. | British Library Conference Proceedings | 1997


    Halpha Surges in Emerging Flux Regions as an Evidence of Magnetic Field Reconnection

    Kurokawa, H. / Sano, S. / International Council of Scientific Unions | British Library Conference Proceedings | 2000