Alfvénic heating in the cusp ionosphere-thermosphere
The effect of electromagnetic variability on cusp-region ionosphere-thermosphere heating is examined. The study is motivated by observed correlations between anomalous thermospheric density enhancements at F region altitudes and small-scale field-aligned currents, previously interpreted as evidence of ionospheric Alfven resonator modes. Height-integrated and height-dependent heating rates for Alfven waves incident from the magnetosphere at frequencies from 0.05 to 2 Hz and perpendicular wavelengths from 0.5 to 20 km have been calculated. The velocity well in Alfven speed surrounding the F region plasma density maximum facilitates energy deposition by slowing, trapping, and intensifying resonant waves. The Alfvenic Joule heating rate maximizes at the resulting resonances. F region Joule heating resulting from quasistatic and Alfvenic variability with the same root-mean-square amplitude in the F region are shown to be comparable. At the same time, Alfvenic variability deposits little electromagnetic power in the E region, whereas quasistatic variability greatly enhances E region heating. When measured electric and magnetic fields are used to constrain the amplitude and spectral content of superposed Alfven waves incident from the magnetosphere, the calculated F region heating rate ranges from 5 to 10 nW/m(2).
document
https://n2t.org/ark:/85065/d7bk1gc6
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2018-12-01T00:00:00Z
Copyright 2018 American Geophysical Union.
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