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Effects of X2-class solar flare events on ionospheric GPS-TEC and radio waves over Brazilian sector

机译:X2级太阳耀斑事件对巴西电离层GPS-TEC和无线电波的影响

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摘要

In this investigation, we present and discuss the effects of 6 X2-class solar flare events in the ionospheric F region over Brazilian sector that occurred during 2013 to 2015. For this investigation, we present the vertical total electron content (VTEC) observations from nearly 120 Global Positioning System (GPS) receivers all over the Brazilian sector for each event. Also, ionospheric sounding observations obtained in Sao Jose dos Campos (23.2 degrees S, 45.9 degrees W, dip latitude 17.6 degrees S; hereafter referred to as SJC), under the southern crest of the equatorial ionospheric anomaly (EIA), Brazil, are presented. The observations show that the greatest TEC impact occurs with the EUV fluxes increases lasting for more than one hour and when the solar active region is located close to the solar disc center. We present a detailed study of the efficiency of the EUV flux with wavelengths ranging from 0.1 to 190 nm for the F region ionization. The largest increase of Delta TEC occurs below the magnetic equator line, covering mainly the central, northeast, southeast and south regions, which includes the equatorial ionospheric anomaly (EIA) region. The ionograms show partial or total fade out in the echoes traces observed causing blackouts of radio signals of up to 60 min, which can have serious consequences to technological systems of public and private agencies around Brazilian sector. This study can help to better understand the effects of solar flares in the ionospheric F region. (C) 2019 COSPAR. Published by Elsevier Ltd. All rights reserved.
机译:在这项研究中,我们介绍并讨论了2013年至2015年发生在巴西电离层F区的6个X2类太阳耀斑事件的影响。对于本次调查,我们提出了近乎垂直的总电子含量(VTEC)观测结果每次活动,巴西各地有120个全球定位系统(GPS)接收器。此外,还介绍了在巴西圣何塞·多斯坎普斯(南纬23.2度,南纬45.9度,倾角17.6度;以下简称SJC)获得的电离层测深观测资料。 。观察结果表明,随着EUV通量的增加持续超过一小时,并且当太阳活动区域位于太阳盘中心附近时,TEC的影响最大。我们对F区电离的EUV通量的效率进行了详细研究,其波长范围从0.1到190 nm。 Delta TEC的最大增加发生在磁赤道线以下,主要覆盖中部,东北部,东南部和南部地区,其中包括赤道电离层异常(EIA)地区。电离图显示,回波痕迹中部分或全部消失,导致最长60分钟的无线电信号停电,这可能会对巴西部门的公共和私人机构的技术系统造成严重影响。这项研究有助于更好地了解电离层F区太阳耀斑的影响。 (C)2019 COSPAR。由Elsevier Ltd.出版。保留所有权利。

著录项

  • 来源
    《Advances in space research》 |2019年第11期|3586-3605|共20页
  • 作者单位

    ITA, Div Ciencias Fundamentais, Sao Jose Dos Campos, Brazil;

    ITA, Div Ciencias Fundamentais, Sao Jose Dos Campos, Brazil;

    ITA, Div Ciencias Fundamentais, Sao Jose Dos Campos, Brazil;

    ITA, Div Ciencias Fundamentais, Sao Jose Dos Campos, Brazil;

    Inst Fed Educ Ciencia & Tecnol Sao Paulo IFSP, Campus Jacarei, Jacarei, SP, Brazil;

    NARL, Gadanki, India;

    Univ Vale Paraiba UNIVAP, Lab Fis & Astron, Sao Jose Dos Campos, SP, Brazil;

    INPE, Sao Jose Dos Campos, SP, Brazil;

    UNLP, Fac Ciencias Astron & Geofis, La Plata, Buenos Aires, Argentina;

    ITA, Div Ciencias Fundamentais, Sao Jose Dos Campos, Brazil;

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

    Solar flare; Ionosphere; GPS; Ionosonde;

    机译:太阳耀斑;电离层;GPS;离子探空仪;

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