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  • 1
    Electronic Resource
    Electronic Resource
    Features of mass supply and flows related with reconnection in the solar corona (1994)
    Springer
    Space science reviews 70 (1994), S. 161-166 
    Details
    ISSN: 1572-9672
    Keywords: Magnetic Fields ; Prominences ; MHD flows
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Symmetrical broadening in the emission spectral lines is the ultimate observational effect of magnetic reconnection in the solar corona. Reconnection can create plasmas of very different temperatures and, hence, very different electrical conductivities in the corona. The electrodynamical effect of such a mass supply is considered. Electromagnetic expulsion force, different from Parker's well-known magnetic buoyancy force, can effectively balance gravity in prominences and generate fast vortex flows in the vicinity of fine threads inside prominences. The possibility of observing this effect from SOHO is discussed.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00777860
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