| 主磁场梯度的空间分布和长期变化特征 |
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| 引用本文： | 高国明, 康国发, 白春华, 王天媛. 主磁场梯度的空间分布和长期变化特征[J]. 地球物理学报, 2012, 55(08): 2651-2659, doi: 10.6038/j.issn.0001-5733.2012.08.017 |
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| 作者姓名： | 高国明 康国发 白春华 王天媛 |
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| 作者单位： | 云南大学地球物理系,昆明 650091 |
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| 摘 要： | 根据GUFM1和IGRF11模型,计算1590—2010年主磁场总强度F、水平分量H和磁倾角I三个要素的水平梯度和垂直梯度,分析了它们的空间分布和长期变化特点.结果表明:F和H的垂直梯度与其磁场的空间分布类似,水平方向的梯度以及磁倾角I在3个方向的梯度都与其磁场分布有明显差异.H的3个方向的梯度分布清楚地指示出南磁极的位置.梯度的长期变化表明,北半球磁场梯度漂移缓慢,南半球磁场梯度变化较快.磁倾角的垂直梯度显示,中太平洋负异常周围的正异常在围绕该负异常旋转.近赤道的梯度异常带在60°W附近的转折是由印度洋异常向非洲方向移动所致.
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| 关 键 词： | 主磁场 水平梯度 垂直梯度 空间分布 长期变化 |
| 收稿时间： | 2012-02-07 |
| 修稿时间： | 2012-07-10 |
Characteristics of the spatial distribution and the secular variation of the main geomagnetic field gradients |
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| GAO Guo-Ming, KANG Guo-Fa, BAI Chun-Hua, WANG Tian-Yuan. Characteristics of the spatial distribution and the secular variation of the main geomagnetic field gradients[J]. Chinese Journal of Geophysics (in Chinese), 2012, 55(08): 2651-2659, doi: 10.6038/j.issn.0001-5733.2012.08.017 |
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| Authors: | GAO Guo-Ming KANG Guo-Fa BAI Chun-Hua WANG Tian-Yuan |
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| Affiliation: | Department of Geophysics, Yunnan University, Kunming 650091, China |
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| Abstract: | Based on the GUFM1 and IGRF11 models, we have calculated the horizontal and vertical gradients of three geomagnetic components during 1590—2010, such as the geomagnetic intensity F, the horizontal component H and the declination I. We also analyzed their spatial distribution and the secular variation. The results indicate that the spatial distributions of the vertical gradient of intensity F and horizontal component H are similar to that of their main field, however, the horizontal gradient and the gradients of declination I in three directions are very different from their field distributions. The vertical gradients of H in three directions clearly show the position of the South magnetic pole. The secular variations of the gradient indicate that the anomaly foci of the gradient are drifting more slowly in the northern hemisphere, but faster in the southern hemisphere. And the gradient variations are more drastic in the northern hemisphere than that in the southern hemisphere. The vertical gradient of the declination I is a negative anomaly in the middle Pacific, and the positive anomaly in the neighboring region tends to rotate about this negative one. The turn of the gradient anomaly belt near the equator of 60°W is caused by the movement of the Indian anomaly to the African direction. |
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| Keywords: | Main geomagnetic field Horizontal gradient Vertical gradient Spatial distribution Secular variation |
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