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Mapping of Geomagnetic Cutoff Rigidity of Cosmic Rays during the Main Phase of the Magnetic Storm of November 20, 2003

机译:2003年11月20日磁场磁场主阶段宇宙射线岩岩截止刚度的映射

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摘要

In this work, geomagnetic cutoff rigidities are calculated in a model magnetosphere field on the world latitude-longitude 5 degrees x 15 degrees grid during the main phase of the magnetic storm of November 20, 2003. A decrease in geomagnetic thresholds (R) by up to 1.8 GV as compared to thresholds in the main field is observed in the maximum of the geomagnetic storm at 2000 UT at middle and low latitudes. In the equatorial part, R amounts to 0.5-0.6 GV. It has been found that the global distribution of drops in the cutoff rigidities exhibits a North-South asymmetry, as well as day-night asymmetry. This is expressed by the fact that the R maximum in the daytime sector is observed at a latitude of 40 degrees N in the Northern Hemisphere and 60 degrees S in the Southern Hemisphere. Conversely, the R maximum is observed in the nighttime sector at a latitude of 55 degrees N in the Northern Hemisphere and 45 degrees S in the Southern Hemisphere. Moreover, the maximum R values in the Northern Hemisphere in the daytime sector are higher than in the nighttime sector; in the Southern Hemisphere, the maximum R values in the daytime sector are lower than in the nighttime sector. The observed magnetospheric effects in the global distribution of R seem to be caused by the dominant impact of the partial ring current that develops in the main storm phase.
机译:在这项工作中,在2003年11月20日磁场磁场的主阶段,在世界纬度5度x 15度网格上的模型磁层场中计算了地磁截止刚性。通过缩小的地磁阈值(R)降低与2000 ut在中低纬度的地磁风暴最多观察到主领域的阈值相比,在主领域的阈值相比,达到1.8 GV。在赤道部分中,R的量为0.5-0.6 GV。已经发现,截止刚性的全球滴剂分布呈北方不对称,以及日夜不对称。这表达了在北半球北半球和60摄氏度的纬度下观察到白天部门的最大值。相反,在夜间扇区的夜间部门观察到北半球的纬度和南半球45摄氏度的夜间扇区。此外,白天部门北半球的最大R值高于夜间部门;在南半球,白天扇区中的最大R值低于夜间部门。 r的全球分布中观察到的磁体效应似乎是由在主风暴阶段发生的部分环电流的显性撞击引起。

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  • 来源
    《Geomagnetism and aeronomy》 |2019年第2期|共8页
  • 作者单位

    Russian Acad Sci SPbB IZMIRAN St Petersburg Branch Pushkov Inst Terr Magnetism Ionosphere &

    Radiowav St Petersburg 191023 Russia;

    Russian Acad Sci SPbB IZMIRAN St Petersburg Branch Pushkov Inst Terr Magnetism Ionosphere &

    Radiowav St Petersburg 191023 Russia;

    Russian Acad Sci SPbB IZMIRAN St Petersburg Branch Pushkov Inst Terr Magnetism Ionosphere &

    Radiowav St Petersburg 191023 Russia;

    Russian Acad Sci SPbB IZMIRAN St Petersburg Branch Pushkov Inst Terr Magnetism Ionosphere &

    Radiowav St Petersburg 191023 Russia;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 地球物理学;
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