Numerical modeling of the behavior of super-small-scale irregularities in the ionospheric F2 layer

被引:0
|
作者
Mingalev, O. V. [1 ]
Mingaleva, G. I. [1 ]
Mel'nik, M. N. [1 ]
Mingalev, V. S. [1 ]
机构
[1] Russian Acad Sci, Kola Sci Ctr, Polar Geophys Inst, Apatity 184200, Murmansk Oblast, Russia
基金
俄罗斯基础研究基金会;
关键词
POWERFUL HF RADIOWAVES; REGION IRREGULARITIES; MAGNETOSPHERIC PLASMA; AURORAL-ZONE; WAVES; SCINTILLATION; DYNAMICS; CAVITONS; DENSITY; TROUGH;
D O I
10.1134/S0016793210050117
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
Using a mathematical modeling method, evolutions of super-small-scale irregularities of electron concentration stretched along the geomagnetic field which could be formed in the magnetized ionospheric plasma of the F2 layer both in a natural way and at an artificial impact on it, in particular, during heating experiments, are studied. Evolution in time of the initially formed irregularities of two types having different shape of the cross sections lateral to the magnetic field (types of direct narrow long band and with a circular cross section) is calculated. It is found that such irregularities during times tens of times shorter than the time of the electron free path time spread out and disappear, accomplishing thereby periodic attenuating oscillations. The period of these oscillations can be equal to both the period of Langmuir oscillations of electrons and the period of cyclotron oscillations of electrons depending on the irregularity type and its initial parameters.
引用
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页码:643 / 654
页数:12
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