给出了描写地磁场中海水绕回转体流动诱导的电场的基本方程、边界条件及其计算方法。
The governing equation, its boundary conditions and computing method for the electrical field induced by seawater flow around axis-symmetric body through geomagnetic field have been developed.
针对现有地磁场模型精度偏低、模型边界效应等问题，深入分析了传统补充国际地磁参考场值的缺陷。
Taking aim at lower precision and boundary effect of the current region geomagnetic field model, the shortage of appending the IGRF data to the regional boundary was analyzed deeply.
理论研究与高空探测结果表明，地磁层的边界在太阳风的作用下将发生形变，形成一个水滴式的界面。
Under the action of solar wind, the magnetosphere boundary is generally deformed like a falling water drop. Theoretical investigations as well as space explorations verify this conjecture.
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