The evolution and propagation of solar transients through the heliosphere
There are several different transient structures that propagate in the solar wind, including Coronal Mass Ejections (CMEs), Solar Energetic Particles (SEPs) and Co-rotating Interaction Regions (CIRs). A CME is an explosion of plasma and magnetic field from the Sun’s corona. SEPs are high energy part...
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University College London (University of London)
2015
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.677684 |