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- W2017864884 abstract "The motion of charged particles in a geomagnetic field distorted by the solar wind is examined, using adiabatic theory. It is shown that the drift motion of particles trapped on high L-shells depends strongly on their equatorial pitch angle. Those mirroring near the equator move in on the night side, while those mirroring at low altitudes move out, thus producing a significant Splitting of the L-shell with pitch angle. One consequence is that the very high latitude lines on the day side may contain trapped particles near the equator, but none near the ends of the lines. The opening up of field lines in the geomagnetic tail may be the Controlling factor governing the high-latitude limit of trapping on both the day side and the night side." @default.
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- W2017864884 date "1966-01-01" @default.
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- W2017864884 title "The Motion of Trapped Particles in a Distorted Field" @default.
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- W2017864884 doi "https://doi.org/10.1007/978-94-010-3553-8_35" @default.
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