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1996—2003年大耀斑事件引起的TEC突然增强的统计分析
A Statistical Analysis of SITEC Caused by Intense Solar Flares During 1996—2003
【摘要】 利用1996—2003年期间 GOES 卫星耀斑观测资料和国际 GPS 观测网的 GPS-TEC 资料分析x 级大耀斑事件引起的电离层电子浓度总含量(TEC)的突然增强(SITEC)现象.对 x 射线耀斑等级、耀斑日面位置与 SITEC 的关系进行了分析.结果表明,两者都与 SITEC 现象的强弱有着一定的正相关性.在消除 X 射线耀斑等级、耀斑日面位置对电离层 SITEC 现象的影响后,进而分析了日地距离以及耀斑持续时间对电离层 SITEC 现象的影响.结果表明,日地距离和耀斑持续时间都是影响 SITEC 现象的重要参数,日地距离较近时发生的耀斑事件引起的 SITEC 现象较为强烈.另外,耀斑持续时间越长,SITEC 现象越微弱,但是当耀斑持续时间继续延长时,SITEC 现象的强弱逐渐趋于不再改变,最后在某值附近达到平衡.还对某些没有在电离层中引起明显 SITEC 现象的耀斑事件进行了讨论,发现了这类耀斑的一些特征.
【Abstract】 In this paper,the SITEC phenomena is investigated which were caused by the X-class X-ray solar flares occurred from 1996 to 2003.The TEC data which obtained from a global GPS networkare used to calculate the TEC increment,ΔTEC_f,and the variation rate increment,Δ(dTEC_f/dt),caused by solar flares.It is found that both ΔTEC_f and Δ(dTEC_f/dt)are closely related with theflare’s maximal X-ray flux and its location on the solar disc.After eliminating the effect of themaximal X-ray fluxes and the locations on solar disc of different flares,results showed that thereis a negative relationship between ΔTEC_f and the distance between the Earth and the Sun.Thelarger the distance,the smaller is the ΔTEC_f.Another finding is that △(dTEC_f/dt)correlates withthe duration of the flare.Some characteristics of the flares which cause no obvious SITEC are alsofound.
【Key words】 Solar flares; Total electron content (TEC); Global position system (GPS);
- 【文献出处】 空间科学学报 ,Chinese Journal of Space Science , 编辑部邮箱 ,2005年01期
- 【分类号】P182.52
- 【被引频次】28
- 【下载频次】144