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Evidence linking coronal transients to the evolution of coronal holes
Authors:David F. Webb  Patrick S. MciIntosh  Jerome T. Nolte  Craig V. Solodyna
Affiliation:(1) American Science and Engineering, Inc., 955 Massachusetts Avenue, 02139 Cambridge, Mass., U.S.A.;(2) Space Environment Laboratory, Environmental Research Labs, National Oceanic and Atmospheric Administration, 80302 Boulder, Colo., U.S.A.
Abstract:The positions of X-ray coronal transients outside of active regions observed during Skylab were superposed on Hagr synoptic charts and coronal hole boundaries for seven solar rotations. We confirmed a detailed spatial association between the transients and neutral lines. We found that most of the transients were related to large-scale changes in coronal hole area and tended to occur on the borders of evolving equatorial holes.Skylab Solar Workshop Post-Doctoral Appointee, 1975–1977.
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