极地研究 ›› 1994, Vol. 6 ›› Issue (1): 20-27.

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1989年3月13日磁暴的亚极光区电离层效应

刘瑞源;刘顺林;温波;刘长发   

  • 出版日期:1994-03-30 发布日期:1994-03-30

IONOSPHERIC EFFECTS OF THE MARCH 13,1989 MAGNETIC STORM AT SUBAURORAL REGION

  • Online:1994-03-30 Published:1994-03-30

摘要:

利用南极长城站(62°13′S,58°58′W)频高图和磁照图研究了1989年3月13日磁暴的亚极光区电离层效应。在紧接着磁暴急始后F层的虚高h′F急剧上升,临频f0F2急剧下降,然后出现扩展F并持续几小时。在磁暴主相,电离层出现严重的吸收,但有时仍能观测到h′F的增加和伴随着的f0F2的降低。在磁暴急始后的第二和第三个晚上观测到极光型Es和夜间E层,其峰值电子浓度高达7.5×105el/cm3,文中讨论了造成这些现象的原因。在同一经度扇区的4个电离层站的h′F和f0F2的行为表明,观测站的纬度越高出现的吸收越严重,f0F2呈下降的时间越长。

关键词: 磁暴,电离层,亚极光区

Abstract:

Ionograms and magnetograms at Great Wall (62°13′S,58°58′W),Antarctica,were used to study the sub auroral ionospheric effects of the March 13,1989 magnetic storm.The virtual height of the F region (h′F) increased and the critical frequency(f 0F 2) decreased rapidly just after the storm's sudden commencement(SSC).Then the spread F appeared and lasted about five hours. During the main phase of the magnetic storm the ionosphere encountered severe absorptions,but large enhancements in h′F and associated depressions in f 0F 2 sometimes were still observed.On the second and third nights after the SSC auroral type sporadic E and night E layers were observed,showing peak electron densities as high as 7.5×10 5el cm -3 .The causes of these phenomena are discussed. Behaviours of h′F and f 0F 2 from four ionosonde stations in the same longitude sector ( Great Wall,Port Stanley,Cachoeira Paulista and Fortaleza) show that the higher the station's latitude is, the more severe absorptions occure, and the longer the depressions of f 0F 2 last.