Volume 35 Issue 5
Sep.  2015
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ZHANG Xiangyu, ZHAO Hua. Simulation Of Induced Step-Transient Magnetic Field With A Lunar Homogeneous Model[J]. Journal of Space Science, 2015, 35(5): 525-532. doi: 10.11728/cjss2015.05.525
Citation: ZHANG Xiangyu, ZHAO Hua. Simulation Of Induced Step-Transient Magnetic Field With A Lunar Homogeneous Model[J]. Journal of Space Science, 2015, 35(5): 525-532. doi: 10.11728/cjss2015.05.525

Simulation Of Induced Step-Transient Magnetic Field With A Lunar Homogeneous Model

doi: 10.11728/cjss2015.05.525
  • Received Date: 2014-09-07
  • Rev Recd Date: 2015-02-03
  • Publish Date: 2015-09-15
  • With a homogeneous model of the Moon, the induced magnetic field caused by step-transient disturbation of interplanetary magnetic field is simulated by the electromagnetic induction theory. As the range of conductivity assigned, the variation from step to calm of both the vectors and magnitudes can be obtained with a fixed permeability μ0. Then the magnetic characteristic transient response function, the field components and total field at 3 different points selected in a longitude line can all be given in different conductivities by numerical inverse Laplace transformation. The calculation provides a reasonable result that components perpendicular to the external step-transient field will disappear in a long-enough time, whereas the parallel component will become unity with it. When the external field step varies, the maximum field value which can be detected in the vicinity of the equator and the polar region are 13.65nT and 2.71nT, respectively. The processes of parallel component change are remarkably different in low latitude and polar region. This phenomenon reflects that magnetometers in different sites of lunar surface may lead to different field curves.

     

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