Abstract
Trapped particle population changes associated with solar events are caused by the effects of solar wind discontinuities on the magnetosphere. The most drastic sequence of such time variations occurs during a magnetospheric storm.
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© 1970 D. Reidel Publishing Company, Dordrecht - Holland
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Roederer, J.G. (1970). Trapped Particle Population Changes Associated with Solar Events. In: Manno, V., Page, D.E. (eds) Intercorrelated Satellite Observations Related to Solar Events. Astrophysics and Space Science Library, vol 19. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3278-0_17
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DOI: https://doi.org/10.1007/978-94-010-3278-0_17
Publisher Name: Springer, Dordrecht
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