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High-Altitude Cusp: The Extremely Dynamic Region in Geospace

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Book cover The Magnetospheric Cusps: Structure and Dynamics

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Abstract

The high-altitude dayside cusps (both northern and southern) are extremely dynamic regions in geospace. Large diamagnetic cavities with significant fluctuations of the local magnetic field strength have been observed there. These cusp diamagnetic cavities are always there day after day and are as large as 6 R E. Associated with these cavities are charged particles with energies from 20 keV up to 10 MeV. The intensities of the cusp energetic ions have been observed to increase by as much as four orders of the magnitude when compared with regions adjacent to the cusp which includes the magnetosheath. Their seed populations are a mixture of ionospheric and solar wind particles. The measured energetic ion fluxes in the high-altitude cusp are higher than that in both the regions upstream and downstream from the bow shock. Turbulent electric fields with an amplitude of about 10 mV/m are also present in the cusp, and a cusp resonant acceleration mechanism is suggested. The observations indicate that the dayside high-altitude cusp is a key region for transferring the solar wind mass, momentum, and energy into the Earth’s magnetosphere.

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  1. Center for Space Physics, Boston University, 725 Commonwealth Avenue, Boston, MA, 02215, USA

    Jiasheng Chen & Theodore A. Fritz

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Theodore A. Fritz Shing F. Fung

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Chen, J., Fritz, T.A. (2005). High-Altitude Cusp: The Extremely Dynamic Region in Geospace. In: Fritz, T.A., Fung, S.F. (eds) The Magnetospheric Cusps: Structure and Dynamics. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3605-1_4

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