Ionospheric plasma density irregularities measured by stimulated electromagnetic emission

被引:17
|
作者
Norin, L. [1 ,4 ]
Grach, S. M. [3 ,5 ]
Leyser, T. B. [4 ]
Thide, B. [4 ,6 ]
Sergeev, E. N. [5 ]
Berlin, M. [2 ,7 ]
机构
[1] Uppsala Univ, Dept Phys & Astron, SE-75120 Uppsala, Sweden
[2] Swedish Univ Agr Sci, Dept Plant Biol & Forest Genet, SE-75007 Uppsala, Sweden
[3] State Univ Nizhniy Novgorod, Radiophys Fac, Nizhnii Novgorod 603950, Russia
[4] Swedish Inst Space Phys, SE-75121 Uppsala, Sweden
[5] Radiophys Res Inst, Nizhnii Novgorod 603950, Russia
[6] Vaxjo Univ, LOIS Space Ctr, Vaxjo, Sweden
[7] Skogforsk Forestry Res Inst Sweden, Uppsala, Sweden
基金
瑞典研究理事会; 俄罗斯基础研究基金会;
关键词
D O I
10.1029/2008JA013338
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is well known that ionospheric plasma turbulence can be conveniently generated by controlled injection of powerful high-frequency radio beams from the ground. Irradiation of the ionosphere with such radio waves leads to the formation of plasma density structures, striations, and the generation of secondary electromagnetic radiation, a phenomenon known as stimulated electromagnetic emission (SEE). In this paper we present experimental results of the dependence of SEE on decreasing excitation levels of the striations. In the experiments the frequency of the injected radio beam was varied near the fifth harmonic of the local ionospheric electron gyro frequency. We use the SEE measurements to obtain transverse length scales of the striations involved in the generation of the SEE. Our results show that different spectral features of the SEE display different temporal dynamics, suggesting that they are related to striations with different transverse length scales (1 less than or similar to L-perpendicular to less than or similar to 25 m).
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页数:9
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