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Published in

Wiley, Journal of Geophysical Research. Space Physics, 7(120), p. 5824-5831, 2015

DOI: 10.1002/2015ja020999

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Pathways of F -region thermospheric mass density enhancement via soft electron precipitation: Cusp Thermospheric Heating

This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Data provided by SHERPA/RoMEO

Abstract

The efficiencies of pathways of thermospheric heating via soft electron precipitation in the dayside cusp region are investigated using the coupled magnetosphere-ionosphere-thermosphere model (CMIT). Event-based data-model comparisons show that the CMITmodel is capable of reproducing the thermospheric mass density variations measured by the CHAMP satellite during both quite and active periods. During blackthe 24 Aug 2005 storm event (Kp = 6-) while intense Joule heating rate occurs in the polar cusp region, including soft electron precipitation is important for accurately modelling the F-region thermospheric mass density distribution near the cusp region. blackDuring the 27 Jul 2007 event (Kp = 2-) while little Joule heating rate occurs in the polar cusp region, the controlled CMIT simulations suggest that the direct blackpathway through the energy exchange between soft electrons and thermospheric neutrals is the dominant process during this event, which only has a small effecton the neutral temperature and mass density at 400 km altitude. blackComparisons between the two case studies show that the indirect pathway via increasing the F-region Joule heating rate is a dominant process during the 24 Aug 2005 storm event, which is much more efficient than the direct heating process.