 Article
 Open Access
 Published:
Determination of the 3D distribution of electrical conductivity in Earth’s mantle from Swarm satellite data: Frequency domain approach based on inversion of induced coefficients
Earth, Planets and Spacevolume 65, Article number: 6 (2013)
Abstract
Mapping the threedimensional (3D) electrical conductivity of Earth’s mantle has been identified as one of the primary scientific objectives for the Swarm satellite mission. We present a 3D frequency domain inversion scheme to recover mantle conductivity from satellite magnetic data. The scheme is based on an inversion of time spectra of internal (induced) spherical harmonic coefficients of the magnetic potential due to magnetospheric sources. Time series of internal and external (inducing) coefficients, whose determination is a prerequisite for this formulation, will be available as a Swarm Level2 data product. An iterative gradienttype (quasiNewton) optimization method is chosen to solve our 3D nonlinear inverse problem. In order to make the inversion tractable, we elaborate an adjoint approach for a fast and robust calculation of the data misfit gradient. We verify our approach with synthetic, but realistic time spectra of internal coefficients, obtained by simulating induction due to a realistic magnetospheric source in a 3D conductivity model of the Earth. In these model studies, both shape and conductivity of a largescale conductivity anomaly in the midmantle are recovered very well. The inversion scheme also shows to be robust with respect to noise and is therefore ready to process Swarm data.
1. Introduction
Mapping the threedimensional (3D) electrical conductivity of Earth’s mantle has been identified as one of the primary scientific objectives for the Swarm multisatellite geomagnetic mission (FriisChristensen et al., 2006). An improved knowledge of the mantle conductivity provides an advanced understanding of the mantle’s chemical and physical properties and reflects the connectivity of constituents such as graphite, fluids and partial melt. Global 3D electromagnetic (EM) induction studies can thus provide complementary information to global seismic tomography (e.g. Becker and Boschi, 2002; Romanowicz, 2003), which is used to ascertain the mantle’s bulk mechanical properties.
Regarding the EM technique, only recent improvements in global 3D EM forward modelling and the growth of computational resources have made rigorous 3D EM inversions on a global scale tractable. A few spherical 3D inverse solutions have been developed recently (Koyama, 2001; Kelbert et al., 2008; Tarits and Mandea, 2010; Kuvshinov and Semenov, 2012), providing the first global and semiglobal 3D mantle conductivity models (Fukao et al., 2004; Koyama et al., 2006; Kelbert et al., 2009; Utada et al., 2009; Tarits and Mandea, 2010; Shimizu et al., 2010; Semenov and Kuvshinov, 2012). Recent progress in global 3D forward and inverse modelling is summarized in two review papers by Kuvshinov (2008, 2012).
All mentioned 3D models have been obtained by inverting data from the groundbased global network of geomagnetic observatories, and are based (except for the work of Tarits and Mandea, 2010) on analysis of Cresponses (Banks, 1969). Although differing in details, the recovered global 3D images reveal a substantial level of lateral heterogeneity in the mantle at depths between 410 and 1600 km; conductivity varies laterally by more than one order of magnitude between resistive and conductive regions.
However, bearing in mind that geomagnetic observatories are sparsely and irregularly distributed with large gaps in oceanic regions and the southern hemisphere, an interpretation of the 3D inversion results in many regions requires extreme care. A lack of observations precludes any conclusive inferences about conductivity distributions in these regions. Moreover, in spite of continuing efforts to improve the coverage by longterm measurements in those regions (Shimizu and Utada, 1999; Chulliat et al., 2009; Korte et al., 2009; Matzka et al., 2009; Toh et al., 2010; among others), reliable images of 3D variations of mantle conductivity in oceanic regions and as a whole in the southern hemisphere can hardly be obtained at present or in the foreseeable future with the use of groundbased data alone.
In contrast to groundbased data, measurements from lowEarthorbit (LEO) platforms provide an excellent spatial coverage with data of uniform quality. However, to date, all practical inversions of existing satellite data have been for 1D (or at most for 2D) conductivity models (e.g. Constable and Constable, 2004; Kuvshinov and Olsen, 2006; Velímský et al., 2006; Martinec and Velímský 2009; Velímský, 2010). The main reason is that the analysis of satellite data is more challenging than the analysis of observatory data, since LEO satellites move typically with a speed of 7—8 km/s and thus, in reality, measure a mixture of temporal and spatial changes of the geomagnetic field. Another reason is that the orbital configurations of recent single satellite missions (Ørsted, CHAMP and SACC) are far from optimal in the context of 3D mantle conductivity studies.
With the Swarm satellite mission, reliable global images of 3D mantle heterogeneities, especially in regions with poor groundbased coverage, come into reach. The forthcoming mission has prompted the initiation of efforts to develop methodologies for recovering 3D electrical conductivity variations from space. The net results of these coordinated studies supported by ESA are summarized in the report by Kuvshinov et al. (2010). One of the initial ideas was to use the C response formalism to interpret satellite data (Kuvshinov et al., 2006), but benchmarking studies showed that the 3D inversion of satellite Cresponses does not yield satisfactory results (Kuvshinov et al., 2010).
In this paper, we describe an alternative approach, based on an inversion of time spectra of internal (induced) spherical harmonic expansion (SHE) coefficients of the magnetic potential that describes the signals of magnetospheric origin. A necessary condition for this approach is the determination of the time series of these and the corresponding external (inducing) coefficients. Both time series will be available as Swarm Level2 data product from the Comprehensive Inversion (CI, Sabaka et al., 2013), which aims to separate magnetic contributions from various sources (originating in the core, lithosphere, ionosphere, and magnetosphere) in the form of corresponding SHE coefficients. An approach to recover 3D mantle conductivity from these data in time domain is described in the companion paper by Velímský (2013).
In Section 2 of this paper, we outline the equations governing global induction, introduce the theoretical concept that forms the basis of our inversion scheme and formulate an “adjoint” approach to efficiently compute the data misfit gradient. In Section 3, we describe how we implemented the concept numerically. Results obtained in model studies with this implementation are presented in Section 4. In Section 5, we summarize the work and give an outlook on planned future improvements.
2. Theoretical Concept
In this section, we first consider the solution of the EM forward problem, which involves the prediction of the EM fields induced by a given timevarying magnetospheric source in a given conductivity model of the Earth (Section 2.1). We then formulate the inverse problem of conductivity recovery as an optimization problem and introduce the relevant terms in Section 2.2. In order to efficiently compute the gradient of the data misfit, we focus on presenting the concept of an adjoint approach in Section 2.3.
2.1 Sketch of the forward problem
In frequency domain, Maxwell’s equations read
Here, B(r, ϑ, φ) and E(r, ϑ, φ) are magnetic and electric fields, respectively, and j^{ext}(r, ϑ, φ) is an impressed source current, with r, ϑ, and φ being distance from Earth’s centre, colatitude and longitude, respectively. σ (r, ϑ, φ) is the spatial conductivity distribution in the Earth, , and γ_{0} is the magnetic permeability of free space. Note that the dependence of B, E and j^{ext} on angular frequency ω is omitted but implied. Also note that we adopt the Fourier convention
In the sourcefree region above the conducting Earth, but below the magnetosphere, Eq. (1) reduces to ∇ × B = 0. B is thus a potential field and can be written as gradient of the magnetic potential V, i.e.
Equations (3) and (5) combine to Laplace’s equation,
The general solution of Eq. (6) can be represented as sum of external and internal parts, V = V^{ext} + V^{int}, which read
Here, a is Earth’s mean radius, and are the expansion coefficients of the external (inducing) and internal (induced) parts of the potential, and is the spherical harmonic of degree n and order m,
with being the Schmidt quasinormalized associated Legendre polynomial of degree n and order ǀmǀ. Note that in Eqs. (7)–(8), we use different indices for external and internal coefficients to account for the 3D structure. In a 3D Earth model, every external coefficient induces a whole series of internal coefficients , such that
where is a transfer function we refer to as “matrix Qresponse” or “Qmatrix”. Note also that here and in the following, we for simplicity use the conventions
In order to solve the coupled Eqs. (1) and (2) inside the conducting Earth, the impressed current j^{ext} has to be known. Our inducing magnetospheric current can be considered in the form of a spherical harmonic expansion of an equivalent sheet current, which is assumed to flow in a shell at r = a (embedded in an insulator) and produces exactly the external magnetic field B^{ext} = −∇V^{ext} at r = a. For a derivation see e.g. Kuvshinov and Semenov (2012), Appendix G. j^{ext} can then be written as
Here, δ(r −a) is Dirac’s delta function, e_{ r } is the outward unit vector, and ∇_{⊥} is the angular part of the gradient operator.
2.2 Inverse problem
We formulate the inverse problem of conductivity recovery as an optimization problem, i.e. we want to minimize a penalty function ϕ(m, λ) given as
with ϕ_{ d } being the data misfit and λ and ϕ_{ s } being a regularization parameter and a regularization term, respectively.
The data misfit ϕ_{ d } (m) is conventionally written as
where d is the data vector, here composed of the experimental (observed) internal coefficients, m is the model vector, and F is the functional solving the forward problem. The model vector m is composed of the N_{ m } model parameters, which in our case describe the conductivity structure of Earth’s mantle. C_{ d } is the data covariance matrix, and superscript ^{†} denotes hermitian matrix transpose. Usually, C_{ d } is assumed to be diagonal (i.e. to contain only the squared uncertainties of the experimental internal coefficients). Thus, we can rewrite Eq. (14) in the following form:
In this representation, ϕ_{d}(m) is the weighted sum (over all harmonics and a set of frequencies Ω) of the squared differences between experimental (observed) and predicted (modeled) internal coefficients, with the uncertainties serving as weights.
The regularization term ϕ_{ s } (m) is conventionally written as
where C_{ m } is the model covariance matrix, and superscript ^{⊤} denotes matrix transpose. It is often more convenient not to define C_{ m }, but the regularization matrix W, such that . With this definition, we can rewrite Eq. (16) as
W is supposed to smooth the solution, its form depends on the desired level of smoothness and the parameterization of the model.
Due to the nonlinearity and the large size of 3D EM inverse problems, iterative gradienttype methods (e.g. Nocedal and Wright, 2006) are typically the methods of choice. These methods require a computation of the gradient of the penalty function ϕ with respect to the model parameters, i.e.
While the gradient of the regularization term is easily calculated analytically and given by
the calculation of the data misfit gradient is more challenging. The straightforward option—bruteforce numerical differentiation—requires extremely high computational loads and is approximate by nature. A much more efficient and elegant way to rigorously calculate the gradient of the misfit is provided by an adjoint approach, see e.g. Dorn et al. (1999). It allows the calculation of the misfit gradient for the price of only a few additional forward calculations (i.e. numerical solutions of Maxwell’s equations) excited by a specific (adjoint) source. Each inverse problem setting requires the finding of explicit formulas for the adjoint source. In the following subsection, we provide these formulas for our inverse problem formulation, following the general derivation by Pankratov and Kuvshinov (2010).
2.3 Adjoint approach
By differentiating Eqs. (7) and (8) with respect to r and setting r = a, we obtain the external and internal parts of the radial component of the magnetic field at Earth’s surface, respectively:
Since , we can solve these equations for the (predicted) internal coefficients by making use of the orthogonality of the spherical harmonics :
Here, ds = sinϑdϑdφ, r = (r = a,ϑ,φ), the upper asterisk of denotes complex conjugation, and is the squared norm of the spherical harmonic . Note that depends only on the external current source j^{ext}, which can be directly verified from Eqs. (12) and (20). B_{ r }, however, also depends on Earth’s conductivity structure (and thus on m).
Taking the total derivative of the data misfit in Eq. (15) yields
where means real part. Since is given by Eq. (22), the only term left to derive is . We first note that, by taking the derivative of Eq. (22), we obtain
where we define
The critical element in Eq. (24) is the total derivative of the radial component of the magnetic field, dB_{ r }. To investigate this element, let us first define the operator G^{ej} (j^{ext}) as the “electric field solution” of Maxwell’s equations (1)–(2) for the current source j>^{ext}, i.e. E = E^{j} = G^{ej}(j^{ext}). Analogously, the operator G^{bj} (j^{ext}) represents the “magnetic field solution” of Maxwell’s equations (1)–(2). Note that these operators are universal and do not depend on the actual forward engine. In a similar way, we can define G^{eh}(h^{ext}) as the electric field solution of a modified set of Maxwell’s equations for the fictitious “magnetic source” h^{ext},
Let us now consider Maxwell’s equations (1)–(2) in an Earth’s model with infinitesimally changed conductivity σ + dσ, yielding electric and magnetic fields E + dE and B + dB, respectively:
Now subtract Eqs. (1)–(2) from Eqs. (28)–(29):
Using the operators defined above, we can rewrite Eq. (30) as
Note that we neglected the second order quantity dσdE. Equations (32) and (31) constitute a set of Maxwell’s equations for the infinitesimal fields dE and dB excited by the “source” dσG^{ej}(j^{ext}). Using the operator representation a second time, we obtain an expression for dB:
An important property of the operators G^{ej}, G^{eh} and G^{bj} are their reciprocity relations (Pankratov and Kuvshinov, 2010):
where
denotes a complexvalued bilinear scalar product. In a spherical coordinate system,
Making use of reciprocity relation (35) and the definitions above, Eq. (24) can be rewritten in operator form:
where
is a fictitious magnetic source, consisting of radial magnetic dipoles distributed along Earth’s surface with weights that are equal to .
Substituting the last line of Eq. (38) into Eq. (23) yields
with
With the definition of the bilinear scalar product (37), we can use Eq. (40) to obtain the elements of the data misfit gradient:
where E^{u} = G^{eh}(u). This representation implies a model built from elementary volume cells V_{ j } each having a piecewise constant conductivity σ_{ j }. The last term in Eq. (42), ∂σ_{ j }/∂m_{ i }, depends on the model parameterization (cf. Pankratov and Kuvshinov, 2010); note that the Einstein summation convention is implied for j. If the model parameters directly represent the conductivites of each cell, i.e. m_{ i } = σ_{ i }, then ∂σ_{ j }/∂m_{ i } = δ_{ ij }, where δ_{ ij } is Kronecker’s delta. Equation (42) demonstrates the essence of the adjoint approach: in order to calculate the gradient of the data misfit, only one (per frequency) additional forward modeling with excitation by the adjoint source u is required.
3. Numerical Implementation
So far, we presented very general derivations, starting from Maxwell’s equations and ending up with the gradient of the penalty function, which is required in gradienttype inversion schemes. These derivations neither depend on the choice of the forward engine (which solves Maxwell’s equations (1)–(2) for a given conductivity model and a given source) nor on the optimization method used to solve the inverse problem. In this section, we specify the model parameterization and the methods we used for the model studies presented in Section 4. The same implementations are planned to be used to analyse actual data of the Swarm satellite mission.
3.1 Forward computations
For forward computations, the 3D conductivity structure σ is discretized on a regular spherical grid, consisting of n_{ r } × nϑ × n_{φ} cells. The conductivity within each elementary volume cell is constant, thus satisfying the condition imposed by Eq. (42). In order to predict electric and magnetic fields generated both by a current source j^{ext} and by an adjoint source u, we use a contracting integral equation approach (extensively described in the paper by Kuvshinov and Semenov, 2012).
The most expensive part of the forward solution in terms of computational cost is the calculation of Green’s tensors. This has been implemented in an efficient way within the inversion algorithm. Since the Green’s tensors are independent of the 3D model (Kuvshinov and Semenov, 2012), their computation has been isolated from the rest of the forward engine and does not need to be repeated in each iteration of the inversion scheme. A parallelization with respect to frequencies ω ϵ Ω has been implemented for a further acceleration of the calculations.
3.2 Inverse parameterization
The inversion domain is divided into N_{r} layers of possibly variable thicknesses. Since our data are coefficients of the SHE of the magnetic potential, it is most natural to also parameterize the model domain in terms of spherical harmonics, as it has been done previously by e.g. Kelbert et al. (2008). Within each layer, conductivity is thus defined as a finite sum of spherical harmonics up to a cutoff degree L, i.e. the number of model parameters N_{ m } is given by N_{ m } = N_{ r } × (L + 1)^{2}. Note that N_{ r } does not necessarily coincide with the number of laterally heterogeneous layers n_{ r } relevant for forward modeling, as we might only try to resolve the conductivity structure of specific layers.
We first normalize the conductivity of each cell by defining
where c_{a} > 0 and c_{ b } > 0 are chosen such that s ∈ [−1; 1] based on assumptions about minimum and maximum conductivities in the mantle. Note that inverting for s instead of σ also constrains the solution to be positive, since solving Eq. (43) for σ yields
We then write s for each layer as a sum of spherical harmonics,
with p and q being degree and order of the spherical harmonics and being Schmidt quasinormalized associated Legendre polynomials. The model vector m is accordingly composed of the coefficients of the SHE,
Its constituents are easily found by inverting Eq. (45), making use of the orthogonality of the spherical harmonics, i.e.
where is the squared norm of the associated Legendre polynomial .
In order to compute the data misfit gradient, the modeldependent term ∂σ_{ j }/∂m_{ i } needs to be known, cf. Eq. (42). For the model parameterization introduced above, this term is given by
The regularization matrix W introduced in Section 2.2 serves as smoothing operator. Radial smoothing, i.e. regularization across layer boundaries, is applied by a finite difference approximation of the vertical gradient (acting on the respective spherical harmonic coefficients). Within each layer, lateral smoothing consists of down weighting spherical harmonics of higher degrees by multiplication with a factor p^{β}, where β > 0 is chosen independently from the bulk regularization parameter λ. However, tests have shown that a variation of β is essentially equivalent to a variation of λ; thus fixing β to a moderate value, e.g. β = 0.3, avoids a twodimensional exploration of the regularization parameter space. Note that this regularization scheme is similar to the scheme previously presented by Kelbert et al. (2008), who however defined the inverse of W.
3.3 Optimization method
To minimize the penalty function given in Eq. (13), we apply the limitedmemory quasiNewton method (LMQN). This method has become a popular tool to solve large 3D EM inverse problems numerically (e.g. Haber, 2005; Avdeev and Avdeeva, 2009). Our implementation of the method follows Nocedal and Wright (2006). The iterative formula for updating the model vector m is
where H^{(k )} is an approximation to the inverse Hessian matrix, updated at every iteration k, using the limitedmemory BroydenFletcherGoldfarbShanno formula. The step length α^{(k)} is computed by an inexact line search.
4. Model Studies
In order to test the performance of our inversion scheme, we generate synthetic data (i.e. time series of internal coefficients) in a test 3D conductivity model, hereinafter referred to as “target model”, and afterwards recover this model from the data. We introduce the target conductivity model (Section 4.1), describe how we generate the test data (Section 4.2) and finally present the results of our model studies (Section 4.3).
4.1 Target conductivity model
Figure 1 shows the target conductivity model. It consists of a thin surface shell of laterally varying conductance and a layered model, which contains different conductivity anomalies, underneath. The shell conductance is obtained by considering contributions both from seawater and sediments. The conductance of seawater has been taken from Manoj et al. (2006) and accounts for ocean bathymetry, ocean salinity, temperature and pressure. Conductance of the sediments (in continental as well as oceanic regions) is based on the global sediment thicknesses given by Laske and Masters (1997) and calculated by a heuristic procedure similar to that described in Everett et al. (2003). The surface shell is scaled to a thickness of 10 km.
Three local conductors of 0.04 S/m, representing possible mantle plumes and subduction zones, are embedded in a resistive layer of 0.004 S/m that extends from 10 km to 400 km. A deepseated largescale structure with conductivity of 1 S/m, describing a hypothetical regional conductor beneath the Pacific plate, is embedded in a layer of 0.04 S/m that extends from 400 km to 700 km. At depths between 700 km and the coremantle boundary at 2900 km, the target model consists of a uniform conductor of 2 S/m; a perfect conductor representing the core is prescribed beneath. Each spherical sublayer is discretized laterally in 180 × 90 cells of 2° × 2°. Note that the aim of this model is not to mimic the “true” world, but to provide a test model for our retrieval algorithm.
4.2 Generation of the test data set
Hourly mean time series of external coefficients in a geomagnetic dipole coordinate system (up to degree n = 3 and order m = 1) have been obtained by analysis of 4.5 years of observatory data (July 1998–December 2002), details of the derivation are given in Olsen et al. (2006). These time series are depicted in Fig. 2. The procedure to obtain the time series of internal coefficients in large parts follows the general scheme described in Olsen and Kuvshinov (2004) and Kuvshinov and Olsen (2005). Here, we only summarize the key steps, a more extensive description is given in Kuvshinov et al. (2006).

1)
Fourier transformation of the external coefficients .

2)
Simulation of EM induction by spherical harmonic sources , for a set of logarithmically spaced frequencies ω_{ j }, using a numerical solution (Kuvshinov, 2008) based on a contracting integral equation approach (Pankratov et al., 1995).

3)
For each frequency ω_{ j }, recovery of by spherical harmonic analysis of the simulated B_{ r } (k, l ≤ 15).

4)
Spline interpolation of to all frequencies.

5)
Calculation of the time spectra of internal coefficients using Eq. (10).

6)
Inverse Fourier transformation of the recovered .
These data constitute a noisefree input for the 3D inversion. For these noisefree data, the model covariance matrix C_{ d } is represented by the identity matrix. Results of such a test inversion are presented in Section 4.3.
In order to realistically simulate the full processing of Swarm data, we however use and to predict the magnetospheric field at orbit altitudes and observatory locations (with a sampling frequency of 1 Hz). Adding the contributions due to different sources (core, lithosphere and ionosphere) yields the magnetic field at orbit altitudes and observatory locations, which is then analyzed by the CI (Sabaka et al., 2013). The external and internal SHE coefficients of the magnetic potential due to magnetospheric sources recovered by the CI constitute a realistic test data set for our inversion scheme. As mentioned in Section 2.2 (cf. Eq. (15)), we use a diagonal model covariance matrix C_{ d }, containing the squared uncertainties of the internal coefficients , which are also recovered by the CI.
4.3 Inversion results
Recovered time series of and are provided by the CI with a sampling rate of 6 hours. The noisefree data are also resampled to 6 hours, and internal coefficients with k > 5 are omitted in order to have structurally similar datasets. For each dataset, we perform a Fourier transformation of both external and internal coefficient time series and pick a subset of representative periods. Tests showed that optimum results are obtained for a period range between two days and two months. For the tests presented in this study, we used 20 logarithmically spaced periods in the abovementioned range.
We invert these data to recover the conductivity at depths between 10 km and 1000 km. The surface conductance map describing the distribution of land and sea is scaled to a thickness of 10 km and fixed, i.e. we do not try to recover it, as its contribution to the induced field is assumed to be known. The inversion domain consists of five layers, each having a thickness of 200 km (except for the uppermost layer, which has a thickness of 190 km). This stratification intentionally does not coincide with the stratification of the target model (cf. Section 4.1) in order to account for our limited knowledge of the stratification in Earth’s mantle.
For forward modelling, each layer (including the thin surface shell) is discretized in 72 × 36 cells of 5° × 5°. Since our data consist of internal coefficients of degree k ≤ 5, we also choose L = 5 as cutoff degree for the spherical harmonic representation of the conductivity in each layer. Although the maximum degrees of data and model are not strictly correlated, tests showed that higher L generate smallscale artefacts in the inversion results, but do not increase the resolution of the anomalous structures. As we use an iterative solver (cf. Section 3.3), an initial conductivity model is required. This model consists of the laterally heterogeneous surface shell and a 1D section underneath, which has been derived from the data by a 1D inversion algorithm (cf. companion paper by Püthe and Kuvshinov, 2013). The conductivity at depths greater than 1000 km is fixed in subsequent iterations just like the conductivity of the surface shell.
The inversion results are presented in Fig. 3. The first column shows the target model “filtered” by spherical harmonics up to degree 5, thereby representing the most detailed picture we can obtain for each layer with the implemented parameterization. Note that the smallscale anomalies in the upper mantle have disappeared, thus indicating that the resolution of our algorithm is limited to largescale structures (i.e. structures of continental size).
The second column shows the conductivity structure recovered with noisefree data. The shape of the largescale anomaly below the Pacific plate is recovered very well in the layer extending from 400 km to 600 km, and conductivities of both anomaly and background match with the filtered target model. The layers extending from 10 km to 200 km and from 200 km to 400 km coincide perfectly well with the (quasiuniform) filtered target model in this depth range. The same is true for the layer extending from 800 km to 1000 km. The layer extending from 600 km to 800 km samples contributions of two layers of the target model (note the different stratifications). Its conductivity distribution appears very reasonable, since the background has an intermediate conductivity when compared to both layers of the filtered target model, and the Pacific plate anomaly is clearly visible.
The third column shows the conductivity structure recovered with realistic test data, i.e. data provided by the CI, generated by simulating observatory measurements and measurements of the three satellites of the Swarm mission in orbit. The shape of the Pacific plate anomaly is blurred when compared to the results obtained with noisefree data, but its conductivity (as well as the background conductivity) matches with the filtered target model. The recovery of the other layers is very similar to the noisefree case, except for the layer extending from 200 km to 400 km, in which a “ghost effect” of the largescale anomaly is perceptible. This might indicate that the data in the considered period range contain only limited information on the conductivity at shallow depths.
As a “failure case study”, an additional run of the CI was performed using simulated observatory measurements and measurements of the two satellites of the Swarm mission that are supposed to fly sidebyside (Swarm A and B, cf. FriisChristensen et al., 2006). Results are shown in the fourth column of Fig. 3. The recovery of the Pacific plate anomaly is comparable to the previous case with data from all three satellites. The recovered model however contains some artefacts in deeper regions. Since the two sidebyside flying satellites are equivalent to a single satellite for mantle conductivity studies, this result indicates that it is possible to obtain a good estimate of the 3D mantle conductivity structure even with data from the global net of observatories and a single satellite, i.e. also from recent missions as, in particular, CHAMP.
The results presented in Fig. 3 were chosen out of a multitude of results obtained with different regularization parameters λ, cf. Eq. (13). The final result was gained by analysis of the tradeoff curve (Lcurve) relating data misfit ϕ_{ d } and regularization term ϕ_{ s } (Hansen, 1992). Figure 4 shows the Lcurve for the inversion runs using the realistic data set (with data from all three satellites); the results shown in the third column of Fig. 3 correspond to the point for λ = 20 in the “knee” of the Lcurve.
5. Discussion and Conclusions
We have presented a 3D frequency domain inversion scheme to invert satellite magnetic data for global mantle conductivity. The scheme is based on the analysis of time spectra of the internal (induced) coefficients of the SHE of the magnetic potential due to magnetospheric sources. The efficacy of the inversion is achieved by the implementation of a limited memory quasiNewton method and the usage of an adjoint approach to calculate the misfit gradient. Parallelization with respect to frequencies and an efficient implementation of the computation of Green’s tensors further accelerate the calculations. Producing the inversion results presented in this paper only took a few hours on 20 nodes of ETH’s cluster “Brutus”.
We parameterize our model domain in terms of spherical harmonics. This parameterization reflects the nature of the data and allows, compared to a block parameterization, a dramatic reduction of the number of model parameters. This stabilizes the solution, as additional tests have shown. The chosen basis does not permit the recovery of sudden lateral jumps in conductivity (sudden vertical jumps, which are expected to occur in the mantle transition zone, can however be mimicked). But in the considered depth range and due to the diffusive nature of electromagnetic fields, we cannot expect to resolve sudden jumps in conductivity anyway. On the other hand, the chosen parameterization diminishes the number of artefacts in the solution. Considering that with the expected data from Swarm, our algorithm can only resolve structures of continental scale, this advantage outweighs the drawbacks.
The algorithm has been tested by simulating induction due to a realistic magnetospheric source in a realistic 3D conductivity model and recovering this model from the synthetic data. The data consist of internal SHE coefficients up to degree and order 5 at periods between two days and two months. By using noisefree data, an excellent recovery of the shape and conductivity of an anomalous largescale structure at midmantle depths (400 km–700 km) has been shown to be possible, whereas the resolution of more detailed structures is limited by the available data. The conductivity of the anomalous structure could also be recovered very well with realistic data provided by the CI, though its shape is slightly blurred. The information in the data on conductivity at shallow depths appears to be limited. The good recovery of the target model with realistic test data in retrospect justifies our neglect of interdependencies between the experimental internal coefficients of different degrees and orders by using a diagonal data covariance matrix. We however plan to implement and investigate the use of the full data covariance matrix, which can be provided by the CI, before applying our formalism to real data.
The presented tests show that the inversion algorithm is workable and ready to digest Swarm data, and might even yield reliable estimates of the 3D mantle conductivity structure with data from recent single satellite missions and the global net of geomagnetic observatories. Further efforts will thus concentrate on the development of a more flexible (modular) structure of the scheme, allowing e.g. the easy insertion of an alternative optimization scheme, such as nonlinear conjugate gradients. This flexibility might allow the combination of the inversion scheme presented in this study with similar global inversion algorithms using observatory data (Semenov and Kuvshinov, 2012; Koch and Kuvshinov, 2013) and thus permit a more robust recovery of mantle conductivity, especially at shallow depths.
The development of an alternative 3D inverse solution is currently in progress. This alternative scheme is not based on internal coefficients , but on the transfer functions , cf. Eq. (10), and thus independent of the source. Another advantage of this scheme is its applicability to patchy time series. The derivation of the elements of the Qmatrix by multivariate analysis and their inversion for mantle conductivity in a similar framework as presented above will be the topic of a forthcoming publication.
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Acknowledgments
The authors thank Oleg Pankratov and Nils Olsen for discussions on different aspects of the paper. We also thank Mark Everett and an anonymous reviewer for helpful and constructive comments on the manuscript. This work has been supported by the European Space Agency through ESTEC contract No. 4000102140/10/NL/JA, by the Swiss National Science Foundation under grant No. 2000021140711/1, and in part by the Russian Foundation for Basic Research under grant No. 120500817a.
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Key words
 3D electromagnetic induction
 3D inversion
 mantle conductivity anomalies
 frequency domain