Influence of magnetospheric processes on winter HF radar spectra characteristics

被引:13
作者
André, R
Pinnock, M
Villain, JP
Hanuise, C
机构
[1] Univ Toulon & Var, LSEET, CNRS, F-83957 La Garde, France
[2] CNRS, LPCE, F-45071 Orleans, France
[3] British Antarctic Survey, Cambridge CB3 0ET, England
关键词
ionosphere; auroral ionosphere; ionosphere-magnetosphere interactions; plasma convection;
D O I
10.5194/angeo-20-1783-2002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This study investigates further the relationship between regions of the magnetosphere and the characteristics of HF radar Doppler spectra recorded in the ionospheric projection of those regions. It builds on earlier work, which has reported a relationship between the Doppler spectral width and the ionospheric projection of the magnetospheric cusp region, by introducing novel techniques for classifying the Doppler spectra recorded by the SuperDARN radars. We first review the geophysical factors that can condition the characteristics of the autocorrelation function (ACF) data produced by the radars. This leads to a classification scheme of the ACF data which is then applied to a large database compiled from winter data taken by the Northern Hemisphere SuperDARN radars. This statistical study shows that the ACF characteristics are not randomly distributed in space, but rather are spatially organized in the ionosphere. This paper suggests that these regions are ordered primarily by the low energy (approximate to 1 keV) electron precipitation region and the presence of intense ULF wave activity.
引用
收藏
页码:1783 / 1793
页数:11
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