Spatial Variation of the Pre-reversal Enhancement - Model Results

Details Spatial Variation of the Pre-reversal Enhancement - Model Results Spatial Variation of the Pre-reversal Enhancement - Model Results

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsa11a1498f&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SA11A-1498

Physics

1240 Satellite Geodesy: Results (6929, 7215, 7230, 7240), 2400 Ionosphere (6929)

Scientific paper

The pre-reversal enhancement (PRE) is one of the most important phenomena controlling the nighttime ionosphere and the generation of equatorial spread F (ESF), but its causal mechanism is still not fully understood. Radar and satellite observations provide us important but incomplete information about it: radars can only observe local time variations at a specific location, while satellites provide data mainly at a single altitude. The NCAR Thermosphere Ionosphere Mesosphere Electrodynamics General Circulation Model (TIME-GCM) is capable of simulating ionospheric phenomena and the pre-reversal enhancement. In this research, we run the model under moderate solar activity (F10.7=150) and geomagnetic quiet conditions to monitor the variation of ionospheric parameters when the maximum upward drift of the PRE is occurring in the Peruvian longitude (75°W). Since it is a three dimensional model, it can provide us current flows, electric field changes and conductivity variations in Peruvian longitude and also longitudes to the east (after PRE) and west (before PRE). From the results, we are able to picture the spatial variations of the ionosphere surrounding the PRE and to evaluate effects due to wind driven current, the equatorial electrojet, and conductivity gradients. In addition, we evaluate the effects of winds and conductivities separately in the ionospheric E and F regions on the PRE, to understand and diagnose the complex electrodynamic processes.

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