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来自近乎球形海洋的感应磁矩。

Induced magnetic moments from a nearly spherical ocean.

作者信息

Styczinski Marshall J, Harnett Erika M

机构信息

Department of Physics, University of Washington, Box 351560, 3910 15th Ave NE, Seattle, WA 98195-1560, USA.

UW Astrobiology Program, University of Washington, Box 351580, 3910 15th Ave NE, Seattle, WA 98195-1580, USA.

出版信息

Icarus. 2021 Jan 15;354:114020. doi: 10.1016/j.icarus.2020.114020. Epub 2020 Aug 4.

Abstract

The five largest planets all have strong intrinsic magnetic fields that interact with their satellites, many of which contain electrically conducting materials on global scales. Conducting bodies exposed to time-varying magnetic fields induce secondary magnetic fields from movement of eddy currents. In the case of spherically symmetric conducting bodies, matching magnetic solutions at the boundary results in relatively simple relations between the excitation field and the induced field. In this work, we determine the more complicated induced magnetic field from a near-spherical conductor, where the outer boundary is expanded in spherical harmonics. Under the approximations that the excitation field is uniform at a single frequency, the product of wavenumber and radius for the body is large, and the average radius of the body is large compared to the perturbation from spherical symmetry, we find that each spherical harmonic in the shape expansion induces discrete magnetic moments that are independent from the other harmonics in the expansion. That is, simple superposition applies to the magnetic moments induced by each perturbation harmonic. We present a table of the magnetic moments induced by each spherical harmonic up to degree 2 in the perturbed shape. We also present a simple formula by which the induced magnetic field may be evaluated for any arbitrary shape described by expanding the radius of the conducting body in spherical harmonics. Unlike the Earth, many moons in the Solar System are tidally locked to their parent bodies, and many also contain saline, subsurface oceans. Conductive material in these moons is therefore expected to be non-spherical. Accounting for the boundary shape of Europa's ocean will be critical for interpretation of magnetic measurements near the moon, where the effects of quadrupole-and-higher magnetic moments will be most apparent. The results of this work permit magnetic studies considering non-spherical oceans of satellites for the first time.

摘要

五大行星都有强大的固有磁场,这些磁场与它们的卫星相互作用,其中许多卫星在全球范围内都含有导电物质。暴露在时变磁场中的导电体会因涡电流的运动而感应出二次磁场。对于球对称导电体,在边界处匹配磁解会导致激发场和感应场之间有相对简单的关系。在这项工作中,我们确定了来自近球形导体的更复杂的感应磁场,其外边界用球谐函数展开。在激发场在单一频率下是均匀的、物体的波数与半径的乘积很大以及物体的平均半径与球对称扰动相比很大的近似条件下,我们发现形状展开中的每个球谐函数都会感应出独立于展开中其他谐函数的离散磁矩。也就是说,简单叠加适用于每个扰动谐函数感应出的磁矩。我们给出了在扰动形状中直至2阶的每个球谐函数感应出的磁矩表。我们还给出了一个简单公式,通过该公式可以针对通过用球谐函数展开导电体半径来描述的任何任意形状评估感应磁场。与地球不同,太阳系中的许多卫星都被潮汐锁定在它们的母天体上,而且许多卫星还含有含盐的地下海洋。因此,预计这些卫星中的导电物质是非球形的。考虑木卫二海洋的边界形状对于解释该卫星附近的磁测量至关重要,在那里四极及更高阶磁矩的影响将最为明显。这项工作的结果首次允许对考虑卫星非球形海洋的磁学进行研究。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8151/8819694/4fe51becee07/nihms-1771782-f0001.jpg

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