Abstract
Two different classes of geomagnetic activity have long been attributed to particle emission from active solar regions. The occurrence of geomagnetic storms subsequent to large solar flares has been explained by the arrival at earth of material ejected by the flare. Recurrent geomagnetic activity has been interpreted as the effect of persistent streams emitted from long-lived active regions on the rotating sun. Within the past decade, both flare-associated and recurrent disturbances have been directly observed on spacecraft probing interplanetary space. This paper will review and interpret these observations, with major emphasis on the flare-associated phenomena. The role of multiple satellite measurements in studying the propagation and spatial structure of interplanetary disturbances will be considered.
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Hundhausen, A.J. (1970). Solar Wind Disturbances Associated with Solar Activity. 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_8
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DOI: https://doi.org/10.1007/978-94-010-3278-0_8
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