# Assessing the hazard from geomagnetically induced currents to the entire high-voltage power network in Spain

- Joan Miquel Torta
^{1}Email author, - Santiago Marsal
^{1}and - Marta Quintana
^{2}

**66**:87

https://doi.org/10.1186/1880-5981-66-87

© Torta et al.; licensee Springer. 2014

**Received: **28 January 2014

**Accepted: **16 July 2014

**Published: **4 August 2014

## Abstract

After the good results obtained from an assessment of geomagnetically induced currents (GICs) in a relatively small subset of the Spanish power transmission network, we now present the first attempt to assess vulnerability across the entire Spanish system. At this stage, we have only included the power grid at the voltage level of 400 kV, which contains 173 substations along with their corresponding single or multiple transformers and almost 300 transmission lines; this type of analysis could be extended to include the 220-kV grid, and even the 110-kV lines, if more detailed information becomes available. The geoelectric field that drives the GICs can be derived with the assumption of plane wave geomagnetic variations and a homogeneous or layered conductivity structure. To assess the maximum expected GICs in each transformer as a consequence of extreme geomagnetic storms, a post-event analysis of data from the Ebre Geomagnetic Observatory (EBR) during the 2003 Halloween storm was performed, although other episodes coincident with very abrupt storm onsets, which have proven to be more hazardous at these mid-latitudes, were analyzed as well. Preferred geomagnetic/geoelectric field directions in which the maximum GICs occur are automatically given from the grid model. In addition, EBR digital geomagnetic data were used to infer statistical occurrence probability values and derive the GIC risk at 100-year or 200-year return period scenarios. Comparisons with GIC measurements at one of the transformers allowed us to evaluate the model uncertainties.

## Keywords

## Background

Solar-terrestrial physics is a discipline with a long tradition, and many observatories and research groups have been dedicated to this subject for a long time. However, as modern society has become more dependent on technological systems and therefore vulnerable to disturbances in the upper atmosphere and in the interplanetary space near Earth, the focus of this discipline evolved in new and important directions, and it has been renamed as space weather (e.g., Song et al. 2001). Space weather covers the study of the conditions in space that could affect human activity. Phenomena originating in the Sun that can affect human activity include explosive events such as flares and coronal mass ejections. These produce large quantities of energetic particles and solar wind disturbances, which travel through the interplanetary medium and affect the terrestrial environment. This solar activity is cyclical (solar cycle) and reaches a maximum approximately every 11 years.

The event that sparked global interest in this discipline, beyond academia, was the collapse of the power grid in northeastern Canada due to the great geomagnetic storm of 13 March 1989; this event left millions of people without power for 9 h (Bolduc 2002). In October-November 2003, during the declining phase of the next solar cycle, a series of events known as the Halloween storm occurred, and as a result, some new problems in electrical transmission networks were encountered (e.g., there was a blackout in the city of Malmö in southern Sweden (Pulkkinen et al. 2005; Wik et al. 2009)) and several space missions and satellites experienced numerous anomalies (Royal Academy of Engineering 2013). Motivated by the events of 2003, the Committee on Solar and Space Physics (CSSP) of the U.S. National Research Council (NRC) began to consider the need to systematically assess the social and economic impacts of space weather. To establish objectives for this research, the CSSP organized a workshop in Washington, D.C. during May 2008. The conclusions obtained as a result of that meeting can be found in the workshop report (U.S. National Research Council 2008). One of the most obvious conclusions revealed by the historical records is that past space weather events, such as the Carrington event in 1859 (Cliver and Dietrich 2013) and the great geomagnetic storm of May 1921 (Kappenman 2006), have been as much or even more severe than some of the more recent ones; this suggests that such extreme events, although rare, are likely to happen again sometime in the future. As stated in the workshop report, according to a study by the Metatech Corporation, today the occurrence of an event like the 1921 storm would result in large-scale blackouts affecting over 130 million people and would put more than 350 transformers at risk of permanent damage.

Geomagnetic storms caused by disturbances in solar conditions can affect the terrestrial environment including the magnetosphere, ionosphere, and magnetosphere-ionosphere interaction region; such effects are detectable at the surface of the Earth (e.g., Blanch et al. 2013). The highly conductive nature of the ionosphere produces significant current systems in this region, such as the equatorial and auroral electrojets. During disturbed conditions, there is a significant increase in these currents (the auroral electrojet can measure on the order of millions of amps). As these are time-varying, intense induced electric currents appear occasionally in conductors at the Earth's surface. The European Space Agency (ESA) launched the Swarm mission in November 2013 to better understand the magnetic field around Earth. This mission provides opportunities for near real-time *in situ* monitoring of the ionosphere and upper atmosphere (Stolle et al. 2013).

The induced electric currents generated by geomagnetic storms in ground-based technical networks are called geomagnetically induced currents (GICs). Their frequencies are typically in the millihertz range, and thus, they can be considered quasi-direct currents (quasi-dc). These currents can disrupt and damage our technological systems, e.g., by affecting transformers of high-voltage networks in the case of power transmission systems. Specifically, transformer cores can saturate under the effect of GICs by operating in the saturation region of the magnetization curve (*B*-*H*) of the steel core (Molinski 2002; Kappenman 2007). When a large number of transformers experience GIC saturation, the demand for reactive power and the harmonics of the system voltage are significantly increased. Reactive power demands of this magnitude can cause serious changes in the system voltage. At the same time, the change in the size of the ferromagnetic material (magnetostriction) between the saturated and unsaturated states at twice the power frequency produces heat, noise, and mechanical vibration damage (Koen and Gaunt 2002). The transformers may also suffer premature aging due to the effects of GICs. This aging can be detected by measuring the concentration of gas in the transformer oil. The harmful effects of magnetic storms on power grids have been observed both at high latitudes and at low and middle latitudes. Damage has even occurred in electrical networks at latitudes lower than Spain, such as in the case of South Africa during the Halloween storm of 2003 (Gaunt and Coetzee 2007). This event was related to the onset of damage in a 700 MVA transformer and in several smaller power transformers. It has been shown (Torta et al. 2012) that during that event, the amplitude of the variations of the horizontal geomagnetic field and its time derivative (*dB*_{
H
}/*dt*), which is more important for geoelectric field generation, were significantly higher at the Ebre Observatory in Spain than in Hermanus, South Africa. It is therefore prudent that we assess the effects of magnetic storms on the Spanish power network.

## Methods

Modeling efforts for calculating GICs in ground-based technological systems require a determination of the electric field that occurs in connection with a magnetic storm at the Earth's surface and a calculation of the resulting GIC (see Pirjola 2002). The practical calculation includes both a geophysical and an engineering problem because the surface geoelectric field is determined from geomagnetic recordings or from ionospheric-magnetospheric current data (if available) as the first step, and then the GIC flow is calculated under the given geoelectric field using the known topology and resistances of a conductor system.

For the determination of the geoelectric field, we have different possibilities. Going from the most sophisticated to the simplest one, one can choose exact formulas for the calculation of magnetic and electric fields at the Earth's surface due to an auroral electrojet, which include contributions from field aligned currents (e.g., Pirjola and Häkkinen 1991). However, the resulting formulas are complicated and unsuited to real-time calculations. On the basis of the experience obtained by this study, we attempt to use a practical procedure for the real-time calculation of GICs, which would allow organizations to find the best way of configuring the power system to mitigate their impact as fast as possible.

*h*above the Earth's surface, the complex depth is

*h*+ 2

*p*, where

*p*is the complex skin depth related to the surface impedance,

*Z*(Wait 1981; Boteler and Pirjola 1998):

Here *i*, *ω*, and *μ*_{0} are the imaginary unit, the angular frequency, and the vacuum permeability, respectively. Both the complex skin depth and the surface impedance are defined in the frequency domain. As a first approximation to the auroral electrojet, Boteler and Pirjola (1998) derived algebraic expressions for the magnetic and electric fields at Earth's surface due to an infinite line current above the Earth using CIM. They considered two different conductivity models representative of Québec and British Columbia, which are resistive and conductive, respectively. It has been demonstrated that CIM gives a very good agreement with the exact methodology. Although it is a convenient tool for theoretical modeling purposes, it is not the most optimal choice for more operational applications because it was simply derived for a line current above the Earth. However, Pirjola and Viljanen (1991) show that the applicability of CIM is not restricted to the line current case as they extended the use of CIM to a more complicated ionospheric-magnetospheric current system. Pirjola et al. (2000) also show the successful use of CIM for a westward-traveling-surge (WTS) event.

Since the true 3-D ionospheric current system cannot be determined by using ground magnetometer data only, the method of Spherical Elementary Current Systems (SECS) (Amm 1997) can be used to introduce a horizontal equivalent current system, which produces the same magnetic and electric field at the Earth's surface. This method is based on the fact that geomagnetic variations at the Earth's surface can be explained by a horizontal divergence-free current system at the ionospheric level. The amplitudes of the elementary current systems are determined by the inversion technique, by fitting the modeled horizontal field to the measured one, and once the currents are determined, obtaining the electric field at the Earth's surface due to one element is straightforward. Inversion is usually resolved by the singular value decomposition technique because the system is typically underdetermined. Data for just three magnetic observatories have even been reported to have been used in the interpolation process to infer the equivalent ionospheric currents (Caraballo et al. 2013).

*B*must be with respect to

*u*rather than with respect to

*t*:

*x*and

*y*indicate the north and east geographical directions, respectively;

*μ*

_{0}is the permeability of free space; and

*σ*is the Earth's conductivity. The ‘+’ sign on the right-hand side applies to (

*E*

_{ x },

*B*

_{ y }) and the ‘−’ sign to (

*E*

_{ y },

*B*

_{ x }). In contrast, if one considers a layered Earth structure, the surface impedance

*Z*(

*ω*) can be obtained for each angular frequency

*ω*by a recursive formula that determines the impedance at the top of any layer in terms of the impedance at the bottom of the layer (see, e.g., Pulkkinen 2003). The geoelectric field in the time domain is then evaluated by the inverse Fourier transform of

where *B*(*ω*) is the Fourier transform of the magnetic field (e.g., Viljanen et al. 2006). The integral in Equation 2 can be easily obtained numerically (Viljanen and Pirjola 1989). In evaluating that integral in practice, the lower limit of integration of Equation 2 is set to *t-M*, where *M* is the amount of time taken into account before *t* (for which the electric field is required). If this interval is sufficient, the time-dependent method (valid for a uniform Earth) provides the same results as the spectral method (valid for the layered Earth) provided that all the layers are given the same conductivity.

**I**) flowing into the Earth (or into the grid) at each of the

*n*nodes. They can be summarized in the following equation:

where **1**, **Y**, and **Z** are the identity matrix, the *n* x*n* network admittance (related with the line resistances) matrix, and the earthing impedance (related with the earthing resistances) matrix, respectively; the *n*-element vector **J** contains information on the electric field computed, as described before, from geomagnetic observatory data.

**Y**and

**Z**matrices are computed according to (Lehtinen and Pirjola 1985)

*R*

_{ ij }is the line resistance between nodes

*i*and

*j*, and if the nodes are far apart,

where *R*_{
i
}^{
e
} is the resistance through which the node *i* is earthed. Pirjola (2008a, b) demonstrated that accounting for the off-diagonal elements of this matrix can be only relevant when the distances between the stations are on the order of hundreds of meters or less. In the Spanish 400-kV network described in the next section, only three node links are separated by less than 500 m (between approximately 350 and 450 m), so all the off-diagonal elements of the earthing impedance matrix were set equal to zero. In any case, neglecting all off-diagonal elements of **Z** is in general less important for the knowledge of the expected GICs than the uncertainties produced by the different approximations and assumptions adopted because it is not always possible to get precise values for all the circuit elements.

**J**vector in Equation 4 is given by

*V*

_{ ij }is the geovoltage from node

*i*to node

*j*, which is given by

*d*l is the differential vector path length, and the integration path

*L*

_{ ij }refers to the transmission line from

*i*to

*j*. If E is conservative, the integral in Equation 8 is independent of the path

*L*

_{ ij }from

*i*to

*j*, and

*V*

_{ ij }=

*V*

_{ i }−

*V*

_{ j }, where

*V*

_{ i }and

*V*

_{ j }are the values of the scalar potential of the geoelectric field at nodes

*i*and

*j*. A particular case of a conservative field is when it can be considered spatially constant in the region of analysis. Then, the GIC values in each node can be expressed in terms of two parameters (

*a*and

*b*), which depend on the geometry and the resistances of the network (and naturally vary from node to node):

In summary, the external (or geophysical) conditions are contained in (*E*_{
x
}, *E*_{
y
}), while the engineering problem is determined by the scalar constants *a* and *b*. Unless one evaluates continental regions (Viljanen et al. 2012), the Earth's curvature can be neglected and planar geometry (rather than spherical) can be used to derive these constants. Horton et al. (2012) even consider the fact that the Earth is not exactly a sphere but an ellipsoid (utilized in global positioning system (GPS) applications that power companies also use).

## Results and discussion

### Data and results

Information relating to the resistances of all the transformers is still incomplete, so that, for simplification, we completely ignored the autotransformers' low-voltage circuits, whereby the winding resistance is the sum of the common and the series resistances. For calculating the total earthing resistance at each substation, we considered the three phases in parallel and added the substation earthing resistance to their equivalent resistance. If the substation is composed of more than one transformer, we assumed that the transformers are connected in parallel and share the same substation earthing resistance. The values of these earthing resistances are in general unknown, but we assumed that they have a typical value of 0.15 Ω (private communication with related power engineers), except for those few substations of the Catalan subset for which we obtained a different value from our previous project. Similarly, in the cases where the resistance of the windings of transformers is unknown, following the criterion of Viljanen et al. (2012), we assumed that *R*_{
i
}^{
e
} takes a typical value of 0.5 Ω, which implies a total resistance for three parallel windings of 0.35 Ω, or 1.05 Ω for one winding. The phase resistances of the power transmission links were calculated according to the values of the resistance per unit length of the conductors at 20°C and the number of conductors per phase supplied by the power company. Then, one must take into account the reduction of three phases into a single conductor.

**Y**and

**Z**matrices computed from the above resistance data allow for the GIC computation at each substation. Accordingly, we obtained a prediction (retrospective in this case) of the GICs in the network nodes and transformers for the Halloween storm and the 24 March 1991 storm, which displayed the most abrupt solar storm commencement at the Ebre Observatory (Torta et al. 2012). We assumed the current network configuration and all elements in operation. Figures 2 and 3 show the resulting GIC in the transformer that we identified as the most vulnerable because it was isolated at the end of a line. On occasion of the abovementioned events, in this transformer, we computed 70 and more than 100 A, respectively. In fact, GICs have been calculated as functions of time through the entire Halloween storm of 29 to 31 October 2003, and the maximum absolute value for each individual substation has been taken and plotted in the map of Figure 4 as circles with diameter proportional to the absolute value of the current. This means that the maxima shown in Figure 4 were not necessarily obtained at the same time point. Large GICs were found in the stations located at the end, or in the corners of transmission lines as intuitively expected and shown by the explicit model calculations for the GIC (e.g., Viljanen and Pirjola 1994; Wik et al. 2008).

Clearly, in a real situation, the geomagnetic field varies in any direction and, consequently, so does the geoelectric field. Thus, the generated GICs will be variable but in proportion to the amplitudes shown in Figures 7 and 8. What is unchanged is the realization, as indicated by Boteler (1994) and Pirjola (2008b), that the GICs are maximized when the incident electric field is in the direction of the bisector of the angle formed by two transmission lines arriving at a substation and minimized in the perpendicular direction. Thus, the transformers at intermediate stations along a long line are not particularly vulnerable to GICs, and therefore, in principle, they are not interesting sites to undertake measurements.

*B*

_{ H }and declination

*B*

_{ D }. Meanwhile, they grouped extreme events that were less than 12 h apart (taking the maximum value for the period) on the grounds that they were part of the same geomagnetic storm event. For each observatory, they computed the peak residual and peak rate-of-change predicted by the observatory GPD to be exceeded within the periods of 100 and 200 years, which was accomplished via the examination of the return-level statistics. The results of Thomson et al. (2011) appear excessively high for the Ebre Observatory compared with those from observatories of similar geomagnetic latitude. This may have happened because the data used still contained artificial peaks in 2001. The predictions made by Thomson et al. (2011) were recalculated after we provided them with geomagnetic data that were reviewed for the period 2000 to 2010 (Table 1); this reanalysis yielded an extreme value of 308 nT/min for

*dB*

_{ H }/

*dt*during the return period of 100 years. This value was used to obtain an approximate size of the GIC magnitudes that would flow in each of the transformers of the grid in the event that the extreme value actually occurred during the return period of 100 years at the Ebre Observatory, and we assumed an impulsive event at a cadence of 1 min along the geomagnetic North (Figure 9). As indicated by Torta et al. (2012), the northward impulse is the most plausible scenario for the most severe events at Ebre Observatory's latitude, where they tend to occur coincident with the abrupt onset of geomagnetic storms.

**The measured maximum and estimated 100-year and 200-year return levels at the Ebre Observatory**

Variable | Measured maximum | 100-year return level | Confidence limit | 200-year return level | Confidence limit | ||
---|---|---|---|---|---|---|---|

| 552 | 706 | 511 | 1,358 | 770 | 534 | 1,509 |

| 112 | 308 | 231 | 384 | 428 | 320 | 535 |

| 0.87 | 1.42 | 0.81 | 2.59 | 1.67 | 0.85 | 3.09 |

| 0.15 | 0.25 | 0.18 | 0.33 | 0.31 | 0.22 | 0.40 |

### Errors by the omission of low-voltage circuits

Horton et al. (2012) provide the calculated GIC results in the network for two geoelectric field scenarios: again, a northward and an eastward uniform electric field of 1 V/km. It was found that we could obtain the same results with our programs. To achieve this, in the case of autotransformers, we had to make use of the concept of virtual nodes (Mäkinen 1993; Pirjola 2005) with an infinite resistance to ground and a resistance of a virtual line between the virtual and the real node equal to the series resistance of the actual autotransformer, while the common resistance is the resistance of the real transformer at the neutral point. Similarly, for full-wound transformers with a Y configuration and grounded both at high- and low-voltage sides, we used an equivalent circuit with two virtual nodes, one in each side of the transformer. Here, again, the virtual nodes have infinite resistances to ground and the virtual line resistances have been set between the virtual and real nodes equal to the real resistances of the transformer windings. Meanwhile, the actual transformer winding resistance was set to zero because it was located at the neutral point of the full-wound transformer.

**Comparison of the total GICs flowing in the ground grid of each substation**

Name | GIC for northward E field (A) | GIC for eastward E field (A) | GIC for northward E field, HV only (A) | GIC for eastward E field, HV only (A) | GIC for northward E field (% diff.) | GIC for eastward E field (% diff.) |
---|---|---|---|---|---|---|

Sub 3 | 139.85 | −109.49 | 131.33 | −185.03 | 6.1 | 69.0 |

Sub 4 | 19.98 | −124.58 | 29.66 | −139.94 | 48.4 | 12.3 |

Sub 5 | −279.08 | −65.46 | −172.81 | −126.07 | 38.1 | 92.6 |

Sub 6 | −57.29 | 354.52 | −49.92 | 319.51 | 12.9 | 9.9 |

Sub 7 | 0.00 | 0.00 | 0.00 | 0.00 | 0.0 | 0.0 |

Sub 8 | 60.90 | 134.30 | 61.74 | 131.53 | 1.4 | 2.1 |

**Comparison of the total GICs flowing in the transformer windings**

Name | Winding | GIC for northward E field (A/phase) | GIC for eastward E field (A/phase) | GIC for northward E field, HV only (A/phase) | GIC for eastward E field, HV only (A/phase) | GIC for northward E field (% diff.) | GIC for eastward E field (% diff.) |
---|---|---|---|---|---|---|---|

T2 | HV | 1.75 | −6.94 | 1.65 | −7.77 | 5.8 | 12.0 |

T5 | Common | 23.31 | −18.25 | 21.89 | −30.84 | 6.1 | 69.0 |

T6 | HV | −9.55 | 59.09 | −8.32 | 53.25 | 12.9 | 9.9 |

T7 | HV | −9.55 | 59.09 | −8.32 | 53.25 | 12.9 | 9.9 |

T8 | HV | −27.67 | −17.89 | −28.80 | −21.01 | 4.1 | 17.5 |

T9 | HV | −27.67 | −17.89 | −28.80 | −21.01 | 4.1 | 17.5 |

T10 | HV | 10.15 | 22.38 | 10.29 | 21.92 | 1.4 | 2.0 |

T11 | HV | 10.15 | 22.38 | 10.29 | 21.92 | 1.4 | 2.0 |

T12 | Common | 0.99 | −8.64 | 3.30 | −15.55 | 232.9 | 80.0 |

T13 | HV | 1.75 | −6.94 | 1.65 | −7.77 | 5.8 | 12.0 |

T14 | Common | 0.99 | −8.64 | 3.30 | −15.55 | 232.9 | 80.0 |

T15 | Common | 23.31 | −18.25 | 21.89 | −30.84 | 6.1 | 69.0 |

### Comparisons with GIC measurements

The best way to evaluate the performance of a model such as the one described here is to compare its predictions at a particular transformer neutral point with actual GIC measurements. This, although planned, is still not possible at key sites such as the transformer at the Manzanares substation. The only measurements coincident with relevant geomagnetic storms were those obtained in 2011 to 2012 on behalf of our previous project (Torta et al. 2012). We do compare here the real observations with the predictions of our new model, including the entire 400-kV Spanish network, for the same transformer named TRP1 (which was wrongly named as TR2 in Torta et al. 2012) at the Vandellòs substation (node 132 in Figure 1) on the occasion of the geomagnetic storm which occurred during 24 to 25 October 2011. Fortunately, there are no autotransformers in this substation, so it is not galvanically interconnected with low-voltage systems and thus we do not expect major errors by ignoring the 220- or 110-kV networks at farther 400-kV stations (Pirjola and Viljanen 1991; Viljanen and Pirjola 1994; Pirjola 2005, 2010).

*σ*= 0.001 S/m (as in Torta et al. 2012) or with different layered conductivity models. For the latter, we chose either the electrical resistivity model given by Pous et al. (1995) for the Ebre basin or the 1-D ground model of the #29 block in Figure 2 by Viljanen et al. (2012). In Table 4, we give the linear correlation coefficients for each case, but in our opinion, this measure is not always the best indicator for quantifying the goodness of such model performances. This is because models that provide the same signal but are amplified several times will provide the same correlation coefficients. Thus, to evaluate how well the model fits the GIC observations, we define the performance (

*P*) parameter as

*σ*

_{ o }is the standard deviation of the set of observations and RMSD

_{ om }is the root mean square deviation of the residuals (or differences between model predictions and observations). Here, the

*o*

_{ i }and

*m*

_{ i }are the

*i*th observation and model output, respectively (or equivalently, those corresponding to time

*t*

_{ i }), from a total of

*N*. Given that the quotient in Equation 10 is a positively defined quantity,

*P*cannot be greater than 1, which is reached when the residuals are zero, i.e., when the model exactly fits the observations. Otherwise,

*P*< 1.

*P*would be 0, for example, for a flat model output equal to the mean of the observations. A negative value of

*P*usually (though not necessarily) denotes anti-correlation. So, in summary, models that perform better have higher values of

*P*, and one can think of

*P*(with some reservations) as the fraction of the standard deviation of the observations that can be explained by the model. Results for this parameter are also given in Table 4 for each of the conductivity case structures tested. None of the proposed 1-D conductivity structures performed substantially better than the homogenous Earth approach, which suggests, as expected, that the actual structure must be laterally heterogeneous, especially because the lateral conductivity contrast is large at ocean-land interfaces (Beggan et al. 2013; Püthe and Kuvshinov 2013); this makes the 1-D assumption probably invalid in the coastal area.

**Quantification of the goodness of different model predictions**

Since the calculated GIC at one site is slightly sensitive to changes made at distant points of the network (Pirjola 2009), our results can be reasonably compared with those presented in Figure 6 by Torta et al. (2012), when only a subset of the grid was modeled. It is well known that the load and operating procedure of the grid change over time. When we prepared our previous model, we did not have the exact elements of maintenance conditions (switched off) for the occasion of the geomagnetic storm, so we had to resort to the state of the grid that happened on a particular day about 3 months later, in which the lines Ascó (node 13 in Figure 1)-Pierola (node 98), Vandellòs (node 132)-Pierola (node 98), and Vandellòs (node 132)-Rubí (node 107) were switched off. Now, *Red Eléctrica de España* has provided us with updates regarding the elements of maintenance during 24 to 25 October 2011. The first important realization was that, on that occasion, one of the transformers at Vandellòs was switched off so that the total current produced by the geomagnetic storm could not be shared among the two transformers at that substation; hence, it only flew through the neutral point of the TRP1 transformer. This explains why the predictions of Torta et al. (2012) were underestimated and they had to artificially decrease the ground conductivity to match the amplitudes of measured and modeled GICs. However, although the overall amplitudes of the present study agree with more realistic conductivity values, our present results correlate worse with the measures of Torta et al. (2012). There are two explanations for this. The first one lies in the fact that Torta et al. (2012) used the time-domain integral approach to infer the electric field from the geomagnetic variation data by setting *M* equal to just 30 min. This converted the data into a surprising result because one would expect that the spectral method or the time-domain method with a sufficiently high *M* should give a better fit for the GIC data (in this study, we used values of *M* around 300 min, which yielded results similar to the spectral method). Using *M* = 30 means that Torta et al. (2012) truncated the impulse response to include only fast variations (i.e., high frequencies). This, in combination with the Earth model that is perhaps not exactly correct, happened to lead to a good fit with measured GIC data (R. Pirjola, D. Boteler, personal communication). A second explanation is related to the topology of the grid in the vicinity of the measuring substation. Besides the second transformer at Vandellòs, the switched off elements in the present model just included the Vandellòs-Rubí transmission line (other switched off elements far apart are not prone to influence the currents at Vandellòs). If we omit again the Vandellòs-Pierola line, the correlation significantly improves (Table 4, last row). We suspect that, although not reported, this transmission line or the Vandellòs-Garraf (node 51 of Figure 1) line, which runs almost parallel, was not operating for at least some time during the storm.

## Conclusions

There is no doubt that space weather effects are an emerging natural hazard, which can have incredibly important effects on our lives, which are marked by increasing levels of technological dependence. They are in the category of high-impact, low-frequency event risks. When space weather effects refer to induced currents in technological systems such as power transmission grids, they are called geomagnetically induced currents, or simply, GICs. Modeling efforts require a determination of the electric field occurring in connection with a magnetic storm at the Earth's surface. There are several possible ways to accomplish this task. Once the geoelectric field is obtained, one can calculate the resulting GIC in the conductor system after obtaining a dc model of it. This engineering task requires knowledge of the geometrical configuration of the network stations and their connections, and also the resistance values of the whole system.

This paper provides much useful information about the expected GIC values in the entire Spanish 400-kV power transmission network, which enables us to conduct an assessment of the vulnerability from that hazard. The network contains 165 substations, to which we added 8 substations from France, Portugal, and Morocco across the respective borders. This represents a complex circuit with 375 transformers and 300 transmission lines. After obtaining the electrical network model to evaluate the maximum expected GIC in each transformer as a result of extreme geomagnetic storms, we developed a post-event analysis from the geomagnetic data obtained at the Ebre Observatory during certain storms, such as the Halloween storm in 2003. We also analyzed other episodes coincident with very abrupt sudden storm commencements, as they have proven to be even more dangerous in mid-latitudes. We found, as expected, that the most susceptible substations to GICs are those in corners or edges of the network. A typical case is that of the Manzanares station which, by having a single transformer, makes it particularly vulnerable. Had the storm of 24 March 1991 occurred with the current network configuration and with all the elements operative, GICs would exceed 100 A in the neutral point of the transformer. However, this extreme value will surely be significantly reduced when transmission lines that are under construction join Manzanares with another station to the east and become operational.

Assessing the vulnerability of a system to GIC hazards usually does not require knowledge of the precise values of expected GICs, instead rough magnitude estimates are sufficient (Pirjola 2008a). However, substantial improvements in our enterprise could be attained with further insights. A clear source of uncertainty in the obtained results arises from the fact of having completely ignored the low-voltage circuits that are galvanically connected to the 400-kV system through autotransformers. This was done because we had neither information on the 220 kV network nor the separate value of the common and series winding resistances of these autotransformers. The 110-kV grid obviously does not have a very big effect on the GIC in the 400-kV system since the lower the voltage, the higher the transmission line resistances, which makes the GICs smaller. The importance of the omission of the low-voltage network has been demonstrated through a test under a GIC benchmark network that has been recently developed by Horton et al. (2012).

To test the model performance on a substation close to the location of Ebre Observatory, where the geomagnetic data came from, a homogenous Earth and a couple of 1-D Earth conductivity models have been employed based on the sparse results of magnetotelluric surveys published in the geophysical literature. This could give rise to calculated geoelectric field amplitudes that may be scaled to incorrect values due to the lack of precise ground conductivity data. In the few sites in which GICs have been or will be effectively measured, the two geoelectric components should be given the correct relative weight when the calculated values are fitted to the measured GIC data (Pirjola 2009; Torta et al. 2012), but because the source field is not exactly a plane wave and the real Earth is not homogeneous, we must consider the specific value of proportionality between the GIC and the electric field only as an ‘effective conductivity’ (Viljanen 1998). Therefore, another improvement would be expected after realistically modeling the induced electric field on the surface of the Earth by using a 3-D model of Earth's conductivity, and this can be done in the manner of recent works such as those by Beggan et al. (2013), Dong et al. (2013), and Püthe and Kuvshinov (2013). In particular, Spain is located on a peninsula, so a precise estimation of the geoelectric field would benefit from modeling the effects of non-uniform conductivities produced by the coast (Gilbert 2005; Thomson et al. 2005; Bürstinghaus et al. 2013; Pirjola 2013).

A critical fact, nevertheless, is the difficulty of obtaining detailed network parameters in the precise instant of a geomagnetic storm and determining the topology of the network for a given amplitude of the incident field. The switching off of a key transmission line or transformer can be essential to boost significant currents through the remaining elements.

## Declarations

### Acknowledgements

This research is part of the project ‘Geomagnetically induced currents in the power transmission network,’ which is funded by Red Eléctrica de España, S.A.U. The GIC measurement data at the Vandellòs substation were obtained by a previous project funded by ENDESA Distribución Eléctrica, S.L. We wish to thank Lluís Serrano, formerly at Ebre Observatory, for preparing most of the software used in this paper, and Ewan Dawson of the Geomagnetism Team, British Geological Survey, Edinburgh, for computing the values provided in Table 1. Some discussions with Risto Pirjola, David Boteler, and Ari Viljanen and their suggestions helped to improve our work. Finally, we wish to acknowledge Risto Pirjola and an anonymous reviewer for their valuable comments and constructive criticisms that greatly enhanced the quality of the manuscript.

## Authors’ Affiliations

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