Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere

Details Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001angeo..19....1s&link_type=abstract

Annales Geophysicae, vol. 19, Issue 1, pp.1-9

Mathematics

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Scientific paper

Solar wind/magnetosheath plasma in the magnetosphere can be identified using a component that has a higher charge state, lower density and, at least soon after their entry into the magnetosphere, lower energy than plasma from a terrestrial source. We survey here observations taken over 3 years of He2+ ions made by the Magnetospheric Ion Composition Sensor (MICS) of the Charge and Mass Magnetospheric Ion Composition Experiment (CAMMICE) instrument aboard POLAR. The occurrence probability of these solar wind ions is then plotted as a function of Magnetic Local Time (MLT) and invariant latitude (7

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