The evolution characteristics of longitudinal magnetic field gradients between photosphere and chromosphere during flares occurring

Details The evolution characteristics of longitudinal magnetic field gradients between photosphere and chromosphere during flares occurring The evolution characteristics of longitudinal magnetic field gradients between photosphere and chromosphere during flares occurring

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994esasp.373...87l&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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