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Observations and modeling of UHF-band scintillation occurrence probability over the low-latitude region of China during the maximum activity of solar cycle 24

机译:太阳周期最大活动期间中国低纬度地区超高频波段闪烁发生概率的观测和建模24

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摘要

The climatological characteristics of UHF-band scintillations over the low-latitude region of China were investigated by analyzing the observations recorded at three stations of our regional network of satellite-beacon-based scintillation monitoring in 2013. The three stations are Hainan (geographic 20.0 degrees N, 110.3 degrees E; geomagnetic 10.1 degrees N, 177.4 degrees W, dip 28.2 degrees), Guangzhou (geographic 23.0 degrees N, 113.0 degrees E; geomagnetic 13.1 degrees N, 174.8 degrees W, dip 33.9 degrees) and Kunming (geographic 25.6 degrees N, 103.7 degrees E; geomagnetic 15.7 degrees N, 176.4 degrees E, dip 39.0 degrees), located at low latitudes of China. The variations of UHF-band scintillation occurrence with latitude, time and season are presented in detail to understand the morphology and climatology of ionospheric scintillations over the low-latitude region of China. An equinoctial asymmetry in the occurrences of scintillation and an obvious difference of the onset time of scintillations between Hainan and Kunming is noted in this data set. Subsequently, the ionosonde data are utilized to study the possible causes of the asymmetry between two equinoxes. The observations suggest that the mean critical frequency (foF2) at 20: 00 LT (12: 00 UT) in the autumnal equinoctial months (September and October) and the vernal equinoctial months (March and April) has a similar asymmetry. The ratio of the mean foF2 between two equinoxes is proportional to the ratio between the maximum scintillation occurrence in the autumnal equinox and in the vernal equinox. Therefore, this ratio can act as a proxy for the equinoctial asymmetry in the occurrences of scintillation over the low-latitude region of China, and can be used to model the equinoctial asymmetry in our empirical climatological model of scintillation occurrence probability (CMSOP). The CMSOP can provide the predictions of the occurrences of scintillation over the low-latitude region of China and was validated in this study.
机译:通过分析我们2013年基于卫星信标的闪烁监测区域网络在三个低纬地区记录的观测资料,调查了中国低纬度地区的UHF波段闪烁的气候特征。这三个站是海南(地理20.0度)北,东111.3度;地磁10.1度,西177.4度,倾角28.2度;广州(地理23.0度,北113.0度;地磁13.1度,北174.8度,倾角33.9度)和昆明(地理25.6度)北纬103.7度,地磁北纬15.7度,东经176.4度,倾角39.0度,位于中国低纬度地区。详细介绍了UHF波段闪烁发生的纬度,时间和季节的变化,以了解中国低纬度地区电离层闪烁的形态和气候。在该数据集中记录了海南和昆明之间闪烁发生的等量不对称性和闪烁开始时间的明显差异。随后,将离子探空仪数据用于研究两个春分点之间不对称的可能原因。观察结果表明,在秋季等月(9月和10月)和春季等月(3月和4月)的20:00 LT(12:00 UT)的平均临界频率(foF2)具有相似的不对称性。两个春分点之间的平均foF2的比例与秋季春分点和春季春分点中最大闪烁发生的比例成正比。因此,该比率可以作为中国低纬度地区发生闪烁时的等时不对称性的替代指标,并可以在我们的闪烁发生概率经验气候模型(CMSOP)中模拟等时不对称性。 CMSOP可以提供中国低纬度地区闪烁发生的预测,并在本研究中得到了验证。

著录项

  • 来源
    《Annales Geophysicae》 |2015年第1期|93-100|共8页
  • 作者单位

    Wuhan Univ, Sch Elect Informat, Wuhan 430072, Peoples R China|China Res Inst Radiowave Propagat, Natl Key Lab Electromagnet Environm, Qingdao, Peoples R China;

    China Res Inst Radiowave Propagat, Natl Key Lab Electromagnet Environm, Qingdao, Peoples R China;

    China Res Inst Radiowave Propagat, Natl Key Lab Electromagnet Environm, Qingdao, Peoples R China;

    China Res Inst Radiowave Propagat, Natl Key Lab Electromagnet Environm, Qingdao, Peoples R China;

    China Res Inst Radiowave Propagat, Natl Key Lab Electromagnet Environm, Qingdao, Peoples R China;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Ionosphere; ionospheric irregularities; modeling and forecasting; radio science; ionospheric propagation;

    机译:电离层;电离层不规则性;建模和预报;无线电科学;电离层传播;

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