利用GPS测量极光带的电子含量:对主槽的初步观测和夏季不规则程度的调查

J.K. Hargreaves , C.J. Burns
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引用次数: 10

摘要

1993年6个月期间,利用全球定位系统卫星的传输,从挪威特罗姆瑟或附近的地点监测电离层电子含量。这些资料已用于高纬度电离层的两个重要现象的初步研究:主槽和大不规则现象的发生。在春季期间多次测定了槽的纬度和运动,并与以往的资料进行了比较。最符合的是Collis和Haggstrom(1988)的公式。在大约从夏至到秋分的四个月期间,研究人员调查了大不规则现象的发生率,并确定了其随时间和磁活动的变化。人们发现,夜间的不规则性要比白天大得多,但由于磁场活动的增加,夜间的不规则性也会增强。给出了统计结果。这些不规则现象可能与先前用非相干散射雷达研究的“极光斑点”相同。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Electron content measurements in the auroral zone using GPS: preliminary observations of the main trough and a survey of the degree of irregularity in summer

Ionospheric electron content was monitored from sites in or near Tromsø, Norway, for six months of 1993, using the transmissions from the satellites of the Global Positioning System (GPS). The data have been used for preliminary studies of two important phenomena of the high-latitude ionosphere: the main trough and the incidence of large irregularities. The latitude and motion of the trough were determined on several occasions during the spring period, and the results compared with previous data. Best agreement is with the formula of Collis and Haggstrom (1988). The incidence of large irregularities was surveyed during a four-month period, approximately from the summer solstice to the autumnal equinox, and the variation with time of day and magnetic activity has been determined. It was found that irregularities are considerably larger by night than by day, but that they are enhanced during both periods by increased magnetic activity. Statistical results are presented. It is suggested that these irregularities are the same as the “auroral blobs” previously studied by incoherent-scatter radar.

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