Characteristics of the development of stimulated and spontaneous magnetospheric substorms according to satellite and ground-based data

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Earth Magnetosphere, Magnetic Disturbances, Magnetic Storms, Satellite Observation, Interstellar Magnetic Fields, Nocturnal Variations, Solar Wind

Scientific paper

It is shown that a substorm stimulated by an external disturbance dBz greater than 2 nTl can begin in the case of a magnetic field configuration that is extended only slightly into the tail. For a highly extended configuration, a substorm can develop in the case of slight external disturbances. Five to ten minutes before the substorm commencement, auroral intensity fluctuations can be observed which arise spontaneously. Alternatively, long-period magnetic-field fluctuations can be observed which are excited by a positive offshoot of the Bz component of the IMF.

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