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    In:  Other Sources
    Publication Date: 2011-08-24
    Description: We review two mechanisms which can lend a non-local character to energy transport in the solar atmosphere, heat flux propagating in the form of collisionless electrons, and non-equilibrium ionization of hydrogen driven by ambipolar diffusion. Application of these processes to modelling of the lower transition region and upper chromosphere is considered.
    Keywords: SOLAR PHYSICS
    Type: In: Electromechanical coupling of the solar atmosphere; Proceedings of the OSL Workshop, Capri, Italy, May 27-31, 1991 (A93-39876 15-92); p. 145-153.
    Format: text
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