The evolution of solar wind strahl
Suprathermal electrons are an important kinetic feature of the solar wind; however, their origin and evolution is yet to be fully understood. Suprathermal electrons are divided into two component populations: the field-aligned, beam-like 'strahl' and the approximately isotropic `halo'...
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University College London (University of London)
2018
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.763188 |