A book discussing the structure and dynamics of magnetospheric cusps will mainly interest graduate level scientists working in geophysics and particularly those studying the earths magnetosphere this collection of survey papers forms essential background reading for those studying or planning to study the magnetosphere cusps . Stagnation flow in the cusp region by using a gas dynamics model o heikkila and winningham 1971 and frank 1971showed a high latitude band of low energy particle precipitation with magnetosheath like properties on the dayside at low altitudes which have been accepted as the first evidence to discover the magnetospheric cusp 2. The cusps have traditionally been described as narrow funnel shaped regions that provide a focus of the chapman ferraro currents that flow on the magnetopause a boundary between the cavity dominated by the geomagnetic field ie the magnetosphere and the external region of the interplanetary medium. The magnetospheric cusp structure and dynamics while pip and ps6 are the quasi sinusoidal pulsations associating with magnetospheric substorm in the appropriate period range from 100 to 400 s . The observed multiple cusps may be either explain as the funnel shaped cusp bifurcated or swiveled into a complicated geometry in space or the cusp was shifted position back and forth three times in about two hours interval as if cluster flew through the cusp three times the observed triple cusps prefer a temporal sequence rather
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