Computer Science – Sound
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....92.5896c&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 92, June 1, 1987, p. 5896-5910. NASA-supported research.
Computer Science
Sound
223
Ion Sources, Ionospheric Ion Density, Ionospheric Sounding, Magnetospheric Ion Density, Space Plasmas, Hydrogen Ions, Oxygen Ions, Plasma Layers, Plasmasphere, Positive Ions, Solar Wind
Scientific paper
The ionospheric contribution of the polar wind and cleft ion fountain at energies less than 10 eV has been added to previously measured sources; this total ion outflow has then been used to calculate the resulting ion density in the different internal regions of the earth's magnetosphere: plasmasphere, plasma trough, plasma sheet, and magnetotail lobes. Using estimated volumes for these regions and an ion residence time characteristic of each region, it is found that the observed magnetospheric densities can be attained in all cases with no contribution from the solar wind plasma. In the case of the plasma sheet the ionospherically supplied density is more than enough to match the observations and even suggests an invisible component of low-energy plasma (less than 10 eV) which has never been observed. A detailed comparison between the calculated ionospheric source effects in the plasma sheet and those recently measured by ISEE shows excellent agreement and suggests a direct polar low-energy ion source for the plasma sheet which has remained unmeasured because of spacecraft potential effects. Although the solar wind is clearly the earth's magnetospheric energy source and energetic solar wind ions are observed in the magnetosphere, these calculations suggest the possibility that the ionospheric source alone is sufficient to supply the entire magnetospheric plasma content under all geomagnetic conditions.
Chappell Charles R.
Moore Thomas Earle
Waite H. Jr. J..
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