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Inner Magnetospherepluto.space.swri.eduhttp://www.ucl.ac.uk/mssl/space Inner Magnetospherepluto.space.swri.eduhttp://www.ucl.ac.uk/mssl/space

Inner Magnetospherepluto.space.swri.eduhttp://www.ucl.ac.uk/mssl/space - PDF document

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Inner Magnetospherepluto.space.swri.eduhttp://www.ucl.ac.uk/mssl/space - PPT Presentation

keV over radial distances mv22BAgain assume particles with pitch angles of 90 in the equatorial plane theperturbation due to one gyrating particle is B ID: 375146

keV) over radial distances =mv"2/2B.Again assume

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