太阳耀斑在太阳极小期和极大期对各纬度地磁分量的影响

Benjamin Ikechukwu Ugwu Ernest, Desmond Okechukwu Ugbor, J. U. Agbo
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引用次数: 1

摘要

利用太阳活动最小期(2009年)和最大期(2002年)实测资料,分析了太阳耀斑与地磁H、Z分量的相互依赖性。利用尼日利亚恩苏卡大学基础空间科学中心工作人员建造的电离层突然监测仪(SIDMON)对太阳耀斑进行了识别。然而,由于SIDMON仍处于初级阶段,因此其结果仍得到卫星数据的证实。结果表明,在太阳极小期和太阳极大期,耀斑对地磁H分量有影响,但对地磁Z分量几乎没有影响。这种影响在赤道纬度比在高纬度地区更为明显。SIDMON的结果虽然不太可靠,但令人鼓舞,因此仪器需要大量改进。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On the effects of solar flare on geomagnetic components across all latitudes during solar minimum and maximum
The mutual dependence of solar flare and geomagnetic H and Z components during the period of least (2009) and maximum (2002) solar activity using archived and observed data were examined. Solar flares were identified by sudden ionosphric monitor (SIDMON) constructed by staff of Centre for Basic Space Sciences, University of Nigeria, Nsukka, Nigeria. However, SIDMON results were still confirmed by satellite data since it was still at the rudimentary stage. Results show that during solar minimum and solar maximum solar flare affects the geomagnetic H component but appears to have little or no effect on the Z component across all the latitudes. The effect is pronounced at the equatorial latitude more than at the high latitudes. Results from SIDMON is though not very reliable but encouraging, thus the instrument needs a lot of improvement.
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Scientific Research and Essays
Scientific Research and Essays 综合性期刊-综合性期刊
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6
审稿时长
3.3 months
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