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Observations of the seasonal dependence of the thermal plasma density in the Southern Hemisphere auroral zone and polar cap at 1 R (sub E)
Journal article   Peer reviewed

Observations of the seasonal dependence of the thermal plasma density in the Southern Hemisphere auroral zone and polar cap at 1 R (sub E)

M. T Johnson, J. R Wygant, C Cattell, F. S Mozer, M Temerin and J Scudder
Journal of Geophysical Research, Vol.106, pp.19,023-19,033
09/01/2001
DOI: 10.1029/2000JA900147

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Abstract

Synoptic maps of the thermal plasma density in the auroral zone and polar cap around 1 R (sub E ) altitude are produced from measurements of Polar spacecraft floating potential during 1 year of perigee passes. The densities are accurate to around a factor of 2 in this region of space. These measurements, which provide the first comprehensive maps of the thermal plasma density over the polar cap and auroral oval, show clear variations in plasma density due to solar illumination of the ionosphere. Number density increases by a factor of 5 for illuminated verses nonilluminated ionospheric conditions over the entire auroral oval and polar cap. The maps delineate the global extent of the large-scale auroral density cavity near 70 degrees + or - 5 degrees invariant latitude. These maps further show that the depth of the density cavity is strongly influenced by solar illumination. The minimum average density ( approximately 0.1 cm (super -3) ) occurs in darkness near 1900 magnetic local time. Copyright 2001 by the American Geophysical Union.
Antarctica Ionosphere Remote Sensing Southern Hemisphere auroral zone magnetic field mapping Miscellaneous polar caps satellite methods seasonal variations solar illumination spatial variations thermal plasma density

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