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The position of the cusp is controlled by the solar wind in a similar way as the low altitude cusp.
Interball Tail and Magion-4 have performed more extensive measurements in the high altitude cusp than any previous spacecraft.
The whistler-mode VLF Cerenkov radiation is generated from the electrons below 1 keV at high altitude cusp magnetosphere, where a local electron gyrofrequency is in VLF band.
During this period, the WIND spacecraft was about 213 RE upstream from the Earth, the GEOTAIL was in the post dusk magnetosheath, the INTERBALL-Tail was near the bow shock, and the POLAR traveled in its dayside outbound orbit from the high altitude cusp to the magnetosheath boundary layer.
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A suprathermal proton population not previously described has been detected in the mid-altitude cusp.
For a better understanding the plasma conditions in the low and middle-altitude cusp region the past FREJA wave data results are used to describe typical wave activity detected in the low-altitude cusp region.
The mid-altitude cusp was found to maintain its fine structure over periods of the order of one hour.
We present the results of a two-point study of the topology and dynamics of high-altitude cusp regions under changing interplanetary magnetic field (IMF) direction.
The whistler waves, electron-cyclotron waves, electron-acoustic waves and Langmuir waves have been detected when the spacecraft was crossing the middle-altitude cusp region.
The events were detected in the dayside high-altitude cusp and were associated with a dramatic decrease and large fluctuations in the local magnetic field strength.
The four Cluster spacecraft observed two distinct regions, showing characteristics of a double cusp, during a mid-altitude cusp pass on 7 August 2004.
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