Evolution of bright points, x-ray jets, their physical parameters and magnetic field in and around coronal holes
Coronal holes exhibit a more rigid rotation with respect to the typical differential rotation at photospheric levels, and thus interchange magnetic reconnection happens at coronal hole boundaries. Transient brightenings (i.e. coronal bright points and X-ray jets) in and around coronal holes have bee...
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Queen's University Belfast
2013
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.601662 |