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Latitude-dependence and dispersion of the westward drift in the geomagnetic field
  • ISSN号:0001-5733
  • 期刊名称:《地球物理学报》
  • 时间:0
  • 分类:P318[天文地球—固体地球物理学;天文地球—地球物理学]
  • 作者机构:Chinese Acad Sci, Inst Geol & Geophys, Beijing 100101, Peoples R China
  • 相关基金:This work was supported by the National Natural Science Foundation of China (Grant Nos. 49734140 and 49974014).
中文摘要:

The main geomagnetic field models of IGRF1900-2000 are used to study the latitude-dependence of the westward drift in the main field. The results show that the latitude-dependence exists in the magnetic components with different wavelengths (m=1-10). The global-average westward drift rate of the component of m=1 is 0.189°/a with the maximum of 0.295°/a at latitudes 40°-45°. The compo-nent of m=2 has an average drift rate of 0.411°/a with the maximum of 1.305°/a at latitude -60°. As for the compo-nents with further shorter wavelengths, the drift is generally restricted in a limited latitude range, and has many smaller drift rates. This latitude-dependence of westward drift can not be explained by rigid rotation of the earth’s core. The results of this note also show that there is a negative disper-sion in the westward drift, namely the components of long wavelengths drift faster than those of short wavelengths. This dispersion feature is not in agreement with Hide’s MHD model. It is likely needed t

英文摘要:

The main geomagnetic field models of IGRF1900–2000 are used to study the latitude-dependence of the westward drift in the main field. The results show that the latitude-dependence exists in the magnetic components with different wavelengths (m=1–10). The global-average westward drift rate of the component of m=1 is 0.189°/a with the maximum of 0.295°/a at latitudes 40°–45°. The component of m=2 has an average drift rate of 0.411°/a with the maximum of 1.305°/a at latitude ?60°. As for the components with further shorter wavelengths, the drift is generally restricted in a limited latitude range, and has many smaller drift rates. This latitude-dependence of westward drift can not be explained by rigid rotation of the earth’s core. The results of this note also show that there is a negative dispersion in the westward drift, namely the components of long wavelengths drift faster than those of short wavelengths. This dispersion feature is not in agreement with Hide’s MHD model. It is likely needed to find a new mechanism for explaining the observed feature of dispersion.

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期刊信息
  • 《地球物理学报》
  • 北大核心期刊(2011版)
  • 主管单位:中国科学院
  • 主办单位:中国地球物理学会 中国科学院地质与地球物理研究所
  • 主编:刘光鼎
  • 地址:北京9825信箱
  • 邮编:100029
  • 邮箱:actageop@mail.igcas.ac.cn
  • 电话:010-82998105
  • 国际标准刊号:ISSN:0001-5733
  • 国内统一刊号:ISSN:11-2074/P
  • 邮发代号:2-571
  • 获奖情况:
  • 首届国家期刊奖,第二届国家期刊奖,中国期刊方阵“双高”期刊,第三届中国出版政府奖
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  • 被引量:31618