Imaging coherent backscatter radar observations of topside equatorial spread F

被引:42
作者
Hysell, DL [1 ]
Woodman, RF
机构
[1] Clemson Univ, Dept Phys & Astron, Clemson, SC 29634 USA
[2] Radio Observ Jicamarca, Lima 13, Peru
[3] Inst Geofis, Lima, Peru
关键词
D O I
10.1029/97RS01802
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Multiple baseline interferometric imaging of a large-scale topside spread F depletion has been performed at the Jicamarca Radio Observatory near Lima, Peru. A new imaging technique makes it possible to examine the detailed structure of the scatter from field-aligned irregularities in and around the depletion. A new antenna at Jicamarca, physically separated from the main antenna array, provided very long interferometry baselines up to similar to 94 lambda long for the observations. High-resolution images of coherent backscatter from the radar plume were computed from the interferometry data using the maximum entropy method. These images show that scattering regions with small Doppler velocities lay mainly along the boundary of the depleted region. Meanwhile, regions with high Doppler velocities were located within the depletion itself and could be seen convecting upward through the depleted channel.
引用
收藏
页码:2309 / 2320
页数:12
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