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Title: Kinetic model of auroral plasma formation II: simultaneous multi-satellite ion observations and interpretations. Technical report

Technical Report ·
OSTI ID:6710740

A detailed analysis of ion composition and distribution observed simultaneously by GEOS 2, SCATHA, and ISEE 1 satellites at the initial phases of an injection event in the inner magnetosphere was made. The mean convection electric field observed by GEOS 2 during the data interval was used to determine the space-time variation of a global time-dependent convection electric-field model, which is approximately verified in this report by ISEE 1 plasma flow measurements and by the unusual SCATHA observation of low-energy ions convected from the plalsmasphere cloak region. Theoretical tracing of ion trajectories with the tested electric-field model indicates that multi-satellite observations of keV ion dispersion can be interpreted in terms of a collision/mixing between an injected auroral ion population rich in oxygen with a preinjection population rich in hydrogen and doubly-ionized helium which had previously moved inward from ISEE 1 orbit. The results of this collision/mixing was that ion dispersion signatures afterwards appeared as if they were from a single population, having lost memory of their previous convection history. This is a possible formulation mechanism of the ad hoc injection boundary which is marked only by plasma dispersion signature and not by any other magnetospheric feature.

Research Organization:
Aerospace Corp., El Segundo, CA (USA). Space Sciences Lab.
OSTI ID:
6710740
Report Number(s):
AD-A-175756/6/XAB; TR-0086(6940-05)-4
Country of Publication:
United States
Language:
English