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A finite-element model implemented in the open-source FreeFem++ program is presented, with the aim of introducing students to the calculation of AC losses in superconductors. With this simple approach, students can learn about the critical state model used to describe the macroscopic electromagnetic behavior of superconductors and the importance of several factors influencing the AC losses of superconductors.
In 2007, Prof. A. M. Campbell presented a numerical model for the solution of the critical state in superconductors. The physics behind the model is the force-displacement curve of the flux lines.
In practice, the model solves Faraday’s equation with a current density J which can take values in the interval [−Jc, Jc] and whose sign depends on that of the magnetic vector potential. For simple problems, a single-step calculation can be used for evaluating the cyclic losses of the superconductors, when this is subjected to a transport AC current or an external AC magnetic field. Despite the limitation of the scenarios that can be simulated, students can gain insights in the problem of AC loss calculations of superconductors by means of this simple approach.
Here, we present the implementation of the model in the open-source finite-element software FreeFem++ [2], which can be easily installed as a stand-alone application on different platforms.
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This enables students to run the scripts on their computers also outside the lecture and review the problems at their own pace.
The model aims at calculating the current density and magnetic field distribution in the transverse cross-section of an infinitely long superconductor.
The simulated domain can therefore be limited to two dimensions. Fig. 1 shows the geometry and the mesh of a typical problem: a superconductor of elliptical cross-section surrounded by an air domain. The magnetic flux density has only two components Bx, By , the Fig. 1. Geometry and mesh for the 2D simulation of an elliptical supercon- ductor surrounded by an air domain. current density and magnetic vector potential have only the z component and are therefore scalars. The current density distribution in the superconductor is calculated by solving Faraday’s equation ∇2A = −µ0J where J takes values approximating the transition between +Jc and −Jc or zero: J = Jcerf(−A/Ar).
In, erf is the error function and Ar is a parameter defining the steepness of the transition. In this work, we used Ar = 1× 10−7 Wbm−1. Instead of erf , other functions based on exponential or hyperbolic arctangent can be used. The sign of J is given by the opposite of that of the magnetic vector potential.
An external uniform magnetic field is applied by setting the boundary conditions for A on the outer air boundary. In 2D Cartesian coordinates, B = ∇ × A becomes Bx = ∂A/∂y, By = −∂A/∂y. For example, in order obtain a magnetic field B0 along y, it is sufficient to impose A = −B0x as boundary condition.
In a similar way, a transport current is imposed by setting a constant value for the magnetic vector potential on the
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Magnetic vector potential distribution for a vertical magnetic field of 30mT, obtained with the condition A = −0.03x applied on the outer boundary.
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Magnetic flux density distribution in and around the superconductor for the conditions boundary. The actual value of the current can be calculated in the post-processing. The cyclic losses can be computed by knowing the current density and the magnetic vector potential at the peak of the excitation Ap as (see equation in and equation in for details).
As an example, we show the case of a superconducting tape of elliptical cross-section subjected to a magnetic field of 30mT perpendicular to the major axis of the ellipse. Such magnetic field is obtained by applying the condition A = −0.03x applied on the outer boundary. Fig. 2 shows the distribution of magnetic vector potential, which bends around the superconductor. As a result of the demagnetization effect, the magnetic field in the superconductor is locally higher than the applied one, reaching a maximum value of 78mT, as shown in Fig. 3. A typical current density distribution, with values equal to ±Jc in the regions penetrated by the magnetic field, is shown in Fig. 4. Possible exercises consist in asking the students to run simulations for different cases, as follows:
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Vary the amplitude of the magnetic field and plot the losses as a function of the amplitude. Observe the non- linear dependence and the change of slope (from Q ≈ B3 to Q ≈ B1), occurring when the field fully penetrates the superconductor. Change the orientation of the field by 90° and observe the large change in the losses. Vary the aspect ratio of the ellipse (without changing its area and Jc) and observe its influence on the losses.
The presented finite-element model, implemented in the open-source FreeFem++ program, allows introducing students to calculation of AC losses in superconductors. The students can learn about the influence of the conductor’s geometry and of field orientation on the AC losses, which is an important topic for the design of efficient superconducting applications.
Introducing AC Loss Calculation in Superconductors through the Campbell Model. (2024, Feb 16). Retrieved from https://studymoose.com/document/introducing-ac-loss-calculation-in-superconductors-through-the-campbell-model
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