Comparison of DMSP cross-track ion drifts and SuperDARN line-of-sight velocities

被引:50
作者
Drayton, RA [1 ]
Koustov, AV
Hairston, MR
Villain, JP
机构
[1] Univ Saskatchewan, Inst Space & Atmospher Studies, Saskatoon, SK S7N 0W0, Canada
[2] Univ Texas, William B Hanson Ctr Space Sci, Dallas, TX 75230 USA
[3] CNRS, F-45045 Orleans, France
关键词
ionosphere; ionospheric irregularities; plasma convection; auroral ionosphere;
D O I
10.5194/angeo-23-2479-2005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Cross-track ion drifts measured by the DMSP satellites are compared with line-of-sight SuperDARN HF velocities in approximately the same directions. Good overall agreement is found for a data set comprising of 209 satellite passes over the field of view of nine SuperDARN radars in both the Northern and Southern Hemispheres. The slope of the best linear fit line relating the SuperDARN and DMSP velocities is of the order of 0.7 with a tendency for SuperDARN velocities to be smaller. The agreement implies that the satellite and radar data can be merged into a common set provided that spatial and temporal variations of the velocity as measured by both instruments are smooth.
引用
收藏
页码:2479 / 2486
页数:8
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