Possible ionospheric preconditioning by shear flow leading to equatorial spread F

被引:28
作者
Hysell, DL [1 ]
Kudeki, E
Chau, JL
机构
[1] Cornell Univ, Dept Earth & Atmospher Sci, Ithaca, NY 14853 USA
[2] Univ Illinois, Dept Elect & Comp Engn, Urbana, IL 61801 USA
[3] Inst Geofis Peru, Lima, Peru
基金
美国国家科学基金会;
关键词
ionosphere; equatorial ionosphere; ionospheric irregularities; space plasma physics; waves and instabilities;
D O I
10.5194/angeo-23-2647-2005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Vertical shear in the zonal plasma drift speed is apparent in incoherent and coherent scatter radar observations of the bottomside F region ionosphere made at Jicamarca from about 1600-2200 LT. The relative importance of the factors controlling the shear, which include competition between the E and F region dynamos as well as vertical currents driven in the E and F regions at the dip equator, is presently unknown. Bottom-type scattering layers arise in strata where the neutral and plasma drifts differ widely, and periodic structuring of irregularities within the layers is telltale of intermediate-scale waves in the bottomside. These precursor waves appear to be able to seed ionospheric interchange instabilities and initiate full-blown equatorial spread F. The seed or precursor waves may be generated by a collisional shear instability. However, assessing the viability of shear instability requires measurements of the same parameters needed to understand shear flow quantitatively - thermospheric neutral wind and off-equatorial conductivity profiles.
引用
收藏
页码:2647 / 2655
页数:9
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