Abstract
This paper is a continuation and an extension of our recent work (Deng et al. in Arch Ration Mech Anal 231(1):153–187, 2019) on the identification of magnetized anomalies using geomagnetic monitoring, which aims to establish a rigorous mathematical theory for the geomagnetic detection technology. Suppose a collection of magnetized anomalies is present in the shell of the Earth. By monitoring the variation of the magnetic field of the Earth due to the presence of the anomalies, we establish sufficient conditions for the unique recovery of these unknown anomalies. Deng et al. (2019), the geomagnetic model was described by a linear Maxwell system. In this paper, we consider a much more sophisticated and complicated magnetohydrodynamic model, which stems from the widely accepted dynamo theory of geomagnetics.
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Acknowledgements
The authors would like to express their gratitudes to the anonymous referee for many insightful and constructive comments, which have led to significant improvements on the results and presentation of the paper. The work of Y. Deng was supported by NSF Grant of China No. 11601528, NSF Grant of Hunan Nos. 2017JJ3432 and 2018JJ3622, Innovation-Driven Project of Central South University, No. 2018CX041. The work of H. Liu was supported by the FRG and startup grants from Hong Kong Baptist University, Hong Kong RGC General Research Funds 12302017, 12301218 and 12302919.
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Appendices
Appendix A: Proof of Lemma 2.2
Define
To prove Lemma 2.2, we next make use of (2.14)–(2.16) to conduct the asymptotic analysis with respect to \(k_s\). Denote by \(\Delta _{\partial \Sigma }:=\nabla _{\partial \Sigma }\cdot \nabla _{\partial \Sigma }\). First, from (2.13) one can show that
Next, we derive the inequality
where C is a constant depends only on \(\Sigma \). In fact, for any \(\Psi \in L_T^2(\partial \Sigma )\), by using the Helmholtz decomposition [2, 9], there exists a unique \(u\in H^1(\partial \Sigma )\), \(\int _{\partial \Sigma } u \mathrm{d}s=0\), such that
By integration by parts there holds
where the last inequality is obtained by using the Poincaré inequality (see, for example, [4]). By using (A.1) and (A.2), one thus derives that
Furthermore, from (2.15) one obtains
By substituting (A.5)–(A.6) into (2.14), it holds that
Since \(-\frac{I}{2} + \mathcal {M}^{0}_{\Sigma _c}\) is invertible on \(\mathrm{TH}(\mathrm{div}, \partial \Sigma _c)\), by combining (A.5)–(A.7), one can obtain (2.18), which completes the proof.
Appendix B: Proof of Lemma 2.3
By the continuity of \(\nu \times \mathbf {H}\) across \(\partial \Sigma \) and \(\partial D_{l}\), and using the same notation as that in Appendix A and the jump formulas (2.4) and (2.6), one can show that
holds on \(\partial \Sigma \) and
holds on \(\partial D_l\), \(l=1, 2, \ldots , l_0\). On the other hand, by using the continuity of \(\nu \cdot \mu \mathbf {H}\) across \(\partial \Sigma \) and \(\partial D_{l}\) (see Lemma 3.3 in [16]), one can further show that
holds on \(\partial \Sigma \) and
holds on \(\partial D_l\), where \(\mathcal {K}_{\Sigma ', \Sigma ''}^{k}: L^2(\partial \Sigma ')\rightarrow L^2(\partial \Sigma '')\), \(\Sigma ', \Sigma ''\in \{\Sigma , \Sigma _c, D_1, D_2, \ldots , D_{l_0}\}\), \(k\in \{0, k_s, k_1, k_2, \ldots , k_{l_0}\}\), are defined by
If \(\Sigma '=\Sigma ''\), then \(\mathcal {K}_{\Sigma ', \Sigma '}^k[\varphi ]:=(\mathcal {K}_{\Sigma '}^k)^*\). Similarly, \(\mathcal {A}_{\Sigma ', \Sigma ''}^{k}: \mathrm{TH}(\mathrm{div}, \partial \Sigma ')\rightarrow \mathrm{TH}(\mathrm{div}, \partial \Sigma '')\), is defined by
Furthermore, by using the boundary magnetic field \(\nu \times \mathbf {H}\) on \(\partial \Sigma _c\), one also has
By combining (2.19)–(B.7), along with straightforward calculations and the similar inequality that is deduced in “Appendix A”, one can derive the following estimates sequentially:
where \(l=1, 2, \ldots , l_0\) and \(N_f:=\mathcal {O}(\Vert \Psi _0\Vert _{\mathrm{TH}(\mathrm{div}, \partial \Sigma _c)}+\sum _{l'=1}^{l_0}\Vert \nabla _{\partial D_{l'}}\varphi _{l'}\Vert _{\mathrm{TH}(\mathrm{div}, (\partial D_l)})\), and
Hence
where the operators \(\mathcal {P}_{D_l, \Sigma _c}: \mathrm{TH}(\mathrm{div}, \partial \Sigma _c)\rightarrow \mathrm{TH}(\mathrm{div}, \partial D_l)\), \(l=1, 2, \ldots , l_0\), are defined by
Noting that \((\mathcal {K}_{D_l}^0)^*\) and \(\mathcal {P}_{D_l, \Sigma _c}\mathcal {L}_{\Sigma _c, D_l}^0\) are compact operators on \(L^2(\partial D_l)\), one can prove the invertibility of \(\varsigma _l I -(\mathcal {K}_{D_l}^0)^*+\mathcal {P}_{D_l, \Sigma _c}\mathcal {L}_{\Sigma _c, D_l}^0\) on \(L^2(\partial D_l)\) by following a similar proof of Lemma 2.2 in [14]. In fact, by the Fredholm theory, it suffices to show the uniqueness of a trivial solution to the following integral equation:
Note that there exists only a trial solution to the following system (see Appendix A in [14]):
On the other hand, one can verify that
is also the solution to (B.13). Therefore, one has
Hence \(\Delta _{\partial D_l}\varphi _l=0\), which proves the unique trial solution to (B.12). Note that \(D_l\), \(l=1, 2, \ldots , l_0\) are small inclusions which are disjoint from each, one can prove the unique solvability of (B.10) (see Appendix B in [14]).
Appendix C: Harmonic Representation of Vectorial Spherical Polynomials
In this appendix, we shall represent \(\mathbf {A}_n^m({\hat{\mathbf {x}}})\xi \), where \(\mathbf {A}_n^m({\hat{\mathbf {x}}})\) is defined in (3.10) and \(\xi \in \mathbb {R}^3\), in terms of vectorial spherical harmonic functions. Recall that the vectorial spherical harmonic functions of degree n are composed of \(\mathbf {M}_{n+1}^m({\hat{\mathbf {x}}})\), \(\mathbf {Q}_{n-1}^m({\hat{\mathbf {x}}})\) and \(\mathbf {T}_n^m({\hat{\mathbf {x}}})\), which are defined in (3.2) and (3.3). From (3.10) one has
By vector calculus identity and integration by parts, we have that
Hence, \(\mathbf {A}_n^m({\hat{\mathbf {x}}})\xi \) is a linear combination of the spherical harmonics \(\{\mathbf {N}_{n+1}^m({\hat{\mathbf {x}}})\}\) and \(\{\mathbf {Q}_{n-1}^m({\hat{\mathbf {x}}})\}\). By straightforward computations, one can obtain that
Similarly, one can show that
and
and
Next, for the last two terms in (C.1), using integration by parts, we have
Furthermore, it holds that
In what follows, we define
By combining (C.3)–(C.8) and using (C.1), one thus has
and
By using the elementary result (cf. [23])
one finally obtains
where
and
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Deng, Y., Li, J. & Liu, H. On Identifying Magnetized Anomalies Using Geomagnetic Monitoring Within a Magnetohydrodynamic model. Arch Rational Mech Anal 235, 691–721 (2020). https://doi.org/10.1007/s00205-019-01429-x
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DOI: https://doi.org/10.1007/s00205-019-01429-x