The adequacy of the ionospheric source in supplying magnetospheric plasma

Details The adequacy of the ionospheric source in supplying magnetospheric plasma The adequacy of the ionospheric source in supplying magnetospheric plasma

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jastp..62..421c&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 62, Issue 6, p. 421-436.

Physics

30

Scientific paper

More than 30 years after the prediction of the polar wind outflow from the high latitude ionosphere, the exact magnitude and ultimate fate of the ionospheric plasma supply remains unknown. Estimates made more than a decade ago suggested that the polar ion outflow might well be of sufficient strength to populate the different regions of the Earth's magnetosphere. Direct measurements in the high altitude magnetosphere became possible only with the launch of the Polar spacecraft. The combination of the Thermal Ion Dynamics Experiment and the Plasma Source Instrument has revealed the presence of low energy (<10 eV) ions moving through the polar regions and into the lobes of the magnetotail. These ions would have been invisible to previous un-neutralized satellites because of the high positive spacecraft potentials. Through the use of a recently developed single particle trajectory and energization code, the movement and energy transformation of these measured particles can be estimated. They are found to move into the plasma sheet region and to be energized to typical plasma sheet energies. The magnitude of the flux of the highly variable out-flowing ions mapped to 1000 km altitude is 1 - 3 × 108 ions/cm2 s in agreement with the original estimates. Future observations by the TIDE/PSI instruments will be required to determine the extent of the total ionospheric contribution.

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