Ionization layers observed at middle latitudes by Atmosphere Explorer-C

被引:23
作者
Heelis, RA [1 ]
机构
[1] Univ Texas, William B Hanson Ctr Space Sci, Richardson, TX 75083 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
D O I
10.1016/S1364-6826(98)00153-9
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In the early phases of the Atmosphere Explorer mission the highly elliptical orbit with apogee near 4000 km and perigee near 135 km, allowed altitude profiles of the ion composition to be obtained over limited latitude extents at middle latitudes. Data from consecutive orbits through the mid-latitude ionosphere show the repeated appearance of ionization layers that are distributed in longitude, appearing at the same geographic location but different geomagnetic locations. In this data set the layers appear at dip latitudes as high as 40 degrees and at these locations the magnetic declination can be significant. Examination of the shape of these layers at different longitudes supports the idea that both meridional and zonal winds may play a role in the field-aligned plasma transport that is primarily responsible for their formation. (C) 1999 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:407 / 414
页数:8
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