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The collective gyration of a heavy ion cloud in a magnetized plasma
Authors:N Brenning  C Swenson  M C Kelley  J Providakes  R Torbert
Institution:

* Royal Institute of Technology, S-100 44, Stockholm, Sweden

** Cornell University, Ithaca, NY 14835, U.S.A.

*** MITRE Corp., Burlington Road, Bedford, MA 01730-2028, U.S.A.

Space Science Center — IEOS, University of New Hampshire, Durham, NH 08324, U.S.A.

Abstract:In both the ionospheric barium injection experiments CRIT I and CRIT II, a long-duration oscillation was seen with a frequency close to the gyro frequency of barium and a time duration of about one second. A model for the phenomenon which was proposed for the CRIT 1 experiment is here compared to the results from CRIT II which made a much more complete set of measurements. The model follows the motion of a low-β ion cloud through a larger ambient plasma. The internal field of the model is close to antiparallel to the injection direction vi but slightly tilted towards the self-polarization direction EP = −vixB. As the ions move across the magnetic field, the space charge is continuously neutralized by magnetic-field aligned electron currents from the ambient ionosphere, drawn by the divergence in the perpendicular electric field. These currents give a perturbation of the magnetic field related to the electric field perturbation by ΔEBVa. The model predictions agree quite well with the observed vector directions, field strengths, and decay times of the electric and magnetic fields in CRIT II. The possibility to extend the model to the active region, where the ions are produced in this type of self-ionizing injection experiments, is discussed.
Keywords:
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