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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Modification of the high latitude ionosphere F region by X-mode powerful HF radio waves: Experimental results from multi-instrument diagnostics
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Modification of the high latitude ionosphere F region by X-mode powerful HF radio waves: Experimental results from multi-instrument diagnostics

机译:X模式强大的HF无线电波对高纬度电离层F区的改造:多仪器诊断的实验结果

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摘要

We present experimental results concentrating on a variety of phenomena in the high latitude ionosphere F2 layer induced by an extraordinary (X-mode) HF pump wave at high heater frequencies (f(H) =6.2-8.0 MHz), depending on the pump frequency proximity to the ordinary and extraordinary mode critical frequencies, foF2 and fxF2. The experiments were carried out at the EISCAT HF heating facility with an effective radiated power of 450-650 MW in October 2012 and October-November 2013. Their distinctive feature is a wide diapason of critical frequency changes, when the f(H)/foF2 ratio was varied through a wide range from 0.9 to 1.35. It provides both a proper comparison of X-mode HF-induced phenomena excited under different ratios of f(H)/foF2 and an estimation of the frequency range above foF2 in which such X-mode phenomena are still possible. It was shown that the HF-enhanced ion and plasma lines are excited above foF2 when the HF pump frequency is lying in range between the foF2 and fxF2, foF2 <= f(H) fxF2, whereas small-scale field-aligned irregularities continued to be generated even when exceeded fxF2 by up to 1 MHz and an X-polarized pump wave cannot be reflected from the ionosphere. Another parameter of importance is the magnetic zenith effect (HF beam/radar angle direction) which is typical for X-mode phenomena under f(H)/foF2 > 1 as well as f(H)/foF2 <= 1. We have shown for the first time that an X-mode HF pump wave is able to generate strong narrowband spectral components in the SEE spectra (within 1 kHz of pump frequency) in the ionosphere F region, which were recorded at distance of 1200 km from the HF heating facility. The observed spectral lines can be associated with the ion acoustic, electrostatic ion cyclotron, and electrostatic ion cyclotron harmonic waves (otherwise known as neutralized ion Bernstein waves). The comparison between the 0- and X-mode SEE spectra recorded at distance far from HF heating facility clearly demonstrated that variety of the narrowband spectral structures were only observed under X-mode HF pumping. The potential generation mechanisms of the different narrowband spectral components are discussed. (C) 2015 Elsevier Ltd. All rights reserved.
机译:我们目前的实验结果集中在高纬度电离层F2层中的各种现象上,这些现象是由高频率(f(H)= 6.2-8.0 MHz)下的非常规(X模式)HF泵浦波引起的,具体取决于泵浦频率接近于普通模式和非常规模式的临界频率foF2和fxF2。实验于2012年10月和2013年10月在EISCAT HF加热设备上进行,有效辐射功率为450-650 MW。它们的独特之处在于,当f(H)/ foF2比率在0.9到1.35之间变化。它既提供了在不同比率的f(H)/ foF2下激发的X模HF感应现象的适当比较,又提供了在foF2之上的频率范围的估计,在该频率范围内这种X模现象仍然可能。结果表明,当HF泵浦频率在foF2和fxF2之间时,foF2 <= f(H)fxF2时,在foF2上方会激发HF增强的离子线和等离子体线,而小规模的场取向不规则现象继续即使超过fxF2达1 MHz,也不会产生电离层,而且X极化的泵浦波也不能从电离层反射出来。另一个重要的参数是磁天顶效应(HF波束/雷达角方向),这是f(H)/ foF2> 1以及f(H)/ foF2 <= 1时X模式现象的典型现象。 X模式HF泵浦波首次能够在电离层F区域的SEE光谱(泵浦频率1 kHz内)中产生强的窄带光谱分量,该分量记录在距HF加热点1200 km处设施。观察到的谱线可以与离子声波,静电离子回旋加速器和静电离子回旋加速器谐波(也称为中和离子伯恩斯坦波)相关。在远离HF加热设备的距离处记录的0模式和X模式SEE光谱之间的比较清楚地表明,只有在X模式HF泵浦下才能观察到各种窄带光谱结构。讨论了不同窄带频谱分量的潜在生成机制。 (C)2015 Elsevier Ltd.保留所有权利。

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