The problem of the MG II resonance lines and the constraints on turbulent transport in the upper chromosphere

Details The problem of the MG II resonance lines and the constraints on turbulent transport in the upper chromosphere The problem of the MG II resonance lines and the constraints on turbulent transport in the upper chromosphere

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994esasp.373...47f&link_type=gif

Solar Dynamic Phenomena and Solar Wind Consequences, Proceedings of the Third SOHO Workshop held 26-29 September, 1994 in Estes

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