Propagation to the ground at high latitudes of auroral radio noise below the electron gyrofrequency
Propagation to the ground at high latitudes of auroral radio noise below the electron gyrofrequency
复制标题
低于电子陀螺频率的极光无线电噪声在高纬度地区传播到地面
DOI:
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发表时间:
1995
期刊:
影响因子:
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通讯作者:
R. Horne
中科院分区:
文献类型:
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作者:
R. Horne
The propagation of auroral radio noise at frequencies below the ionospheric electron gyrofrequency (ƒce ≈ 1.4 MHz) at high latitudes is investigated using the HOTRAY ray tracing code. Two mechanisms are described whereby energy in this frequency range may access the ground. It is assumed that the radiation is generated by an upgoing loss cone in regions of depleted electron density above the ionosphere according to the theory of Wu et al. (1989). It is demonstrated that since the waves are generated with ƒpe ƒce in the ionosphere and for a dipole magnetic field, Z mode waves are reflected in the topside ionosphere and do not have access to the ground. However, Z mode waves can access the second radio window where energy can be mode converted into whistler mode waves which do propagate to the ground. Typically, the range of initial wave normal angles is a few degrees and the resulting latitudinal spread of emissions on the ground is a few degrees. This suggests that any emissions observed on the ground should be closely confined in latitude to the generation region. For a density model where ƒpe < ƒce throughout the ionosphere it is shown that Z mode waves can propagate through the ionosphere and hence to the ground for ƒLcut < ƒ < ƒce where ƒLcut is the left-hand cutoff frequency. Due to refraction these waves are spread over a few tens of degrees in latitude but the spread should decrease with decreasing frequency. This suggests there is low-frequency cutoff to this mechanism below which waves can only reach the ground by mode conversion.