Abstract
Recent research into the effects of the interplanetary magnetic field (IMF) on the Earth's auroral oval and plasmapause are reviewed. While the IMF sector structure has been known for some time to produce asymmetries in polar-cap convection, recent work has shown these effects to extend into the dayside auroral oval. A restricted region of local times referred to as the convection ‘throat’ is found to move to either side of the noon meridian in response to changes in the IMF B y component.
The question of the entry of solar-wind plasma into the magnetosphere continues to be a prime area of research. While it is generally felt that magnetic merging must play some significant role, evidence continues to mount that it does not occur at the subsolar magnetopause, as previously supposed, and that other driving forces for antisunward convection must occur on closed field lines. A suggestion is made that many of the seemingly conflicting observations that have been made in the region of the dayside cusps can be explained if significant distortions of closed field lines near the dayside magnetopause are allowed and if closed and open field lines coexist in the cusp, particularly near the entry layer.
Effects of the IMF on the nightside auroral oval and on the plasmapause stem chiefly from the expansion of the oval to lower latitudes which is produced by southward IMF components and from the impulsive substorm phenomena that become stronger and more probable with increasingly southward IMF.
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Proceedings of the Symposium on Solar Terrestrial Physics held in Innsbruck, May–June 1978.
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Burch, J.L. Effects of the interplanetary magnetic field on the auroral oval and plasmapause. Space Sci Rev 23, 449–464 (1979). https://doi.org/10.1007/BF00172250
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DOI: https://doi.org/10.1007/BF00172250