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Quasi3D spectral wavelet method for a thermal quench simulation
Journal of Mathematics in Industry volume 11, Article number: 17 (2021)
Abstract
The finite element method is widely used in simulations of various fields. However, when considering domains whose extent differs strongly in different spatial directions a finite element simulation becomes computationally very expensive due to the large number of degrees of freedom. An example of such a domain are the cables inside of the magnets of particle accelerators. For translationally invariant domains, this work proposes a quasi3D method. Thereby, a 2D finite element method with a nodal basis in the crosssection is combined with a spectral method with a wavelet basis in the longitudinal direction. Furthermore, a spectral method with a wavelet basis and an adaptive and timedependent resolution is presented. All methods are verified. As an example the hotspot propagation due to a quench in Rutherford cables is simulated successfully.
Introduction
A standard finite element method (FE method) allows to discretize and solve differential equations on arbitrary geometries [1]. Attaining a sufficient resolution with a standard threedimensional (3D) FE approach may be intractable within a limited computation time. For certain geometries, however, an adapted discretization and simulation method may reduce the computational expense. This work focuses on multiscale problems featuring domains with a high ratio between the extend in one spatial direction, referred to as longitudinal direction, and the extend in the other spatial directions, referred to as crosssection, which are, moreover, the translationally invariant with respect to the longitudinal direction. If the crosssection requires a high resolution, because it is e.g. very detailed, performing a standard FE method would be computationally very expensive due to a large number of degrees of freedom. Usually, one would remedy this issue by reducing the model to a twodimensional (2D) [2] or even onedimensional (1D) [3] model by exploiting the symmetry planes. Unfortunately, this simplification is no longer possible as soon as the physical behavior breaks the symmetry, e.g. for a longitudinally asymmetrical heat source in a thermal heat conduction problem.
The described configuration occurs in superconducting magnets in particle accelerators. These magnets struggle with the quench phenomenon, which is a sudden and local transition from the superconducting to the normal state [4]. Quenches emerge randomly during continuous operation. The affected regions normally cool down again and return to a superconducting state in doing so. Sometimes, however, a quench leads to a thermal runaway and the magnet can take irreversible damage if protection measures are not taken in time [4]. Sensitive safety margins lead to a high fault time of the accelerator [5]. The further improvement of the protection systems necessitates the study of the transient effects inside the magnet by numerical simulations [6].
An alternative to the FE approach is based on a quasi3D method, that becomes applicable by exploiting the geometrical symmetry of the model [7, 8]. Here, a 2D FE method in the crosssection is combined with a 1D spectral method [9] in the longitudinal direction. While this approach utilizes FE ansatz functions of lowest order, the order of the spectral element ansatz functions is chosen arbitrarily or appropriately for the problem at hand. Hence, the Q3D method is similar to an anisotropic hpmethod [10].
In earlier works, harmonic functions [7] and orthogonal polynomials [8] have been used as basis functions for the spectral method. In this work, however, wavelets and the corresponding scaling functions are used as an alternative to these. A comparison of orthogonal polynomials and wavelets is made. Wavelets are functions that are defined by properties within the multiresolution analysis (MRA) [11]. In this work, the Daubechies wavelets [12] are utilized.
This paper is structured as follows. First, an introduction to wavelets is given and a spectral method using wavelets is derived. Then, the FE method and the spectral wavelet method are combined into a hybrid Q3D method. Next, an adaptive resolution strategy is discussed for the spectral method. Lastly, the methods are compared and employed to compute the heat conduction in a benchmark model representing a superconducting Rutherford cable as used in superconducting accelerator magnets [13, 14], see Fig. 1. Here, the asymmetrical heat excitation generated by a quench is simulated by an artificial heat source. To obtain a realistic quench simulation, a magnetothermal coupling is required, which would necessitate the use of vectorial edge shape functions [15]. These are more involved than nodal ones and beyond this work’s scope [16].
Introduction to wavelets
General statements
The MRA [11] consists of closed spaces \(V_{j}\) that are nested subspaces of each other, i.e. it holds that \(V_{j}\subset V_{j1}\). Furthermore, the spaces \(W_{j}:=V_{j}^{\perp }\cap V_{j1}\) are defined as the orthogonal complement of \(V_{j}\) in \(V_{j1}\). Thus, it holds that
and
for \(i\neq j\). By applying (1) to itself, one gets
where ⊕ denotes the direct sum. There are scaling functions \(\phi _{j,n}\) and wavelets \(\psi _{j,n}\). They are equipped with a scale j and a translation n and are defined as
Within these definitions, the mother scaling function ϕ and the mother wavelet ψ are used. These coincide with the scaling function and wavelet, respectively, for \(j=0\) and \(n=0\).
The scaling functions and wavelets at fixed scale j constitute an orthonormal basis to the space \(V_{j}\) and \(W_{j}\), respectively. To be more precise, it holds that
DaubechiesN kind wavelets
There is a great variety of different kinds of wavelets [12, 17]. However, within the spectral methods of this work, scaling functions and wavelets of the DBN kind are used, because they are compactly supported and constructed in a way to have a maximum number of vanishing moments [12]. To be more precise, the wavelets have a number of N vanishing moments, i.e. it holds
for \(k=0,\dots ,N1\). Moreover, they are constructed such that they have a minimal support width for the given number of vanishing moments [18]. The scaling functions used in this work are continuous for \(N>1\). In [19] one can find estimates for the Hölder regularity for the scaling functions with \(N=2,\dots ,10\). For \(N=2,3,4\), these are also determined in [12]. It follows that the scaling functions are continuously differentiable for \(N=3,4,5\) and two times continuously differentiable for \(N=6,7,8\). The wavelets have the same regularity properties. For \(N=6\), scaling function and wavelet are depicted in Fig. 2.
The differential equations to be solved in the subsequent sections are formulated on intervals. Consequently, for \(N\geq 2\) there are always functions that are partially inside and partially outside the interval. But a basis that is defined on the interval is required. The construction of such a basis as proposed in [20] is used in this work. Let \(I= [a,b ]\) be an interval. For each boundary N boundary scaling functions and boundary wavelets are constructed, such that the number of vanishing moments is preserved. Inside the interval, the ordinary functions are used.
Because the boundary scaling functions and boundary wavelets can be written as a linear combination of scaling functions, they feature the same regularity. For a sufficient small scale j, the scaling functions on the interval I are defined by
Herein, \(\mathcal{D}\) indicates the number of basis functions on the interval and \(\mathcal{J}\) indicates the number of interior basis functions. With this definition, the space of scaling functions at scale j on the interval I can be defined as
The space of wavelets at scale j on the interval I, indicated by \(W^{I}_{j}\), is defined analogously.
Spectral methods with waveletsbases
As stated above, the Q3D methods is a combination of a 2D FE method and a 1D spectral method. The latter one, that uses a waveletbasis, is examined in this section. It is exemplary developed for the 1D heat equation. The partial differential equation (PDE) together with the boundary conditions and the initial condition reads as
with \((x,t)\in \Omega _{\mathrm{t}}\),
Here, x is the spatial coordinate in m, t the time in s, \(\theta (x,t)\) the unknown temperature in K, \(\lambda (x)\) the thermal conductivity in W/(m K), \(c_{\mathrm{V}}(x)\) the volumetric heat capacity in J/(m^{3} K) and \(q(x,t)\) the volumetric heat flux density in W/m^{3}. Furthermore, the problem is defined on the domain \(\Omega _{\mathrm{t}}:=\Omega \times (0,\infty )\), where Ω is the spatial domain. The boundary ∂Ω is divided in \(\Gamma _{\mathrm{dir}}\) and \(\Gamma _{\mathrm{neum}}\), with \(\partial \Omega = \Gamma _{\mathrm{dir}}\cup \Gamma _{\mathrm{neum}}\) and \(\Gamma _{\mathrm{dir}}\cap \Gamma _{\mathrm{neum}}=\emptyset \), on which Dirichlet \(\theta _{\mathrm{dir}}(x,t)\) in K and Neumann boundary conditions \(g_{\mathrm{neum}}(x,t)\) in W/m^{2} are defined, respectively. The initial condition uses the initial value \(\theta _{0}(x)\) in K.
Let for this section be \(\Omega =(0,L)\). The temperature \(\theta (x,t)\) is then approximated by \(\tilde{\theta }(x,t)\) in \(V^{\Omega }_{j}\) for each time instance. The ansatz of method of lines leads to
The Galerkin approach is applied to (2). Therefore, (2) is tested with the basis functions of \(V^{\Omega }_{j}\). With the inner product \((u(x) ,v(x) ):=\int _{\Omega }u(x)v(x) \,\mathrm{d}x\), this leads to
for \(m = 0,\dots ,\mathcal{D}1\). After inserting (3) into (4), one receives the semidiscrete equation
The used components are defined as
where
Integration by parts is used in the calculation of the entries of \(\mathbf{A}^{\mathrm{sf}}_{\lambda }\). For homogeneous material properties, \(\mathbf{M}^{\mathrm{sf}}_{c_{\mathrm{V}}}\) is a diagonal matrix due to the orthonormality of the scaling functions. Consequently, \(\mathbf{M}^{\mathrm{sf}}_{c_{\mathrm{V}}}\) is a regular matrix and (5) is a system of ordinary differential equations.
For the boundary conditions to be satisfied, one can find a matrix \(\mathbf{B}^{\mathrm{sf}}\in \mathbb{R}^{2\times \mathcal{D}}\) and a vector \(\mathbf{b}^{\mathrm{sf}}\in \mathbb{R}^{2\times 1}\) such that the equation
has to hold for every time instance. For discretizing (5) in time, an arbitrary time integration method can be used.
Quasi3D method
Definition of the domain and spaces
The Q3D method shall be derived by means of the 3D heat equation
where \((\mathbf{x},t)\in \Omega _{\mathrm{t}}\). With a 2D and open domain \(\Omega _{\mathrm{S}}\subset \mathbb{R}^{2}\) and \(I=(0,L)\), the spatial domain defined as
extends in zdirection from 0 to L. Moreover, it assumed that the geometry is translationally invariant with respect to the zdirection. The boundary ∂Ω is divided in three different parts
Next the related spaces need to be defined. Let
be the space of polynomial finite elements of order m, where \(\Pi _{m}\) is the set of all polynomials up to order m and \(\mathcal{T}\) is a twodimensional triangulation (see [1]). With this,
Combining the bases of both spaces, \(S_{1}\) and \(V^{I}_{j}\), a basis for \(K^{j}\) is given by
with \(\nu _{m}\in S_{1}\), \(\hat{\phi }_{j,n1}\in V^{I}_{j}\) and \(\mathcal{I}\) being the number of nodes in the triangulation \(\mathcal{T}\). To make the following derivation clearer, the notation
is used to reduce the number of indices from 3 to 2. Thus, the basis for \(K^{j}\) can be written as
Derivation of the Q3D method
The Q3D method is derived for the 3D heat equation (6). The temperature is approximated in \(K^{j}\). Using the ansatz of method of lines leads to
The heat equation is tested with \(\kappa _{j,m}\) for \(m=1,\dots ,\mathcal{D}\mathcal{I}\). Together with (9), one receives the semidiscrete equation
similar to (5). It is assumed that the material parameters can be written as \(\lambda (\mathbf{x}) = \lambda _{xy}(x,y)\lambda _{z}(z)\) and \(c_{\mathrm{V}}(\mathbf{x}) = c_{\mathrm{V},xy}(x,y)c_{\mathrm{V},z}(z)\). Then, the matrices can be written as
and
where ⊗ denotes the Kronecker product. The remaining matrices, i.e. the stiffness matrix of the 2D FE method and mass matrices of the spectral and FE method, are defined as
with
For homogeneous material properties, \(\mathbf{M}^{\mathrm{fe}}_{c_{\mathrm{V}}}\) is symmetric and positivedefinite because of
for \(\boldsymbol{\upxi }\in \mathbb{R}^{\mathcal{I}}\setminus \{ 0 \} \). Thus, \(\mathbf{M}^{\mathrm{fe}}_{c_{\mathrm{V}}}\) is a regular matrix. Because \(\mathbf{M}^{\mathrm{sf}}_{c_{\mathrm{V}}}\) is regular as well, \(\mathbf{M}^{\mathrm{Q3D}}_{c_{\mathrm{V}}}\) is nonsingular due to the properties of the Kronecker product and thus, (10) is a system of ordinary differential equations.
Under the assumption that the volumetric heat flux density can be written as \(q(\mathbf{x},t) = q_{xy}(x,y,t)q_{z}(z,t)\), the right hand side of (10) reads as
with
and
For the realization of the boundary conditions, the three different parts of the boundary, defined in (8a)–(8c), are considered individually. At the front and back side, \(S_{\mathrm{front}}\) and \(S_{\mathrm{back}}\), this is done with the spectral method, and at the hull \(S_{\mathrm{side}}\) with the FE method.
Adaptive resolution
In the spectral method in Sect. 3, scaling functions at the same scale are used for the whole interval as basis functions. Thus, the resolution is constant for the whole interval as well. When considering a very long domain in zdirection, a high resolution becomes computationally very expensive due to the large number of degrees of freedom. With the adaptive resolution method (ARM) derived in this section, a resolution depending on the location is chosen utilizing the wavelet transform, such that the overall accuracy is sufficiently high. This can strongly decrease the required degrees of freedom.
The boundary basis functions (Sect. 2.2) are chosen such that the main properties of wavelets still hold. In particular, it holds that \(V^{I}_{j}\subset V^{I}_{j1}\), \(W^{I}_{j}={V^{I}_{j}}^{\perp }\cap V^{I}_{j1}\) and
This allows to decompose the spaces \(V^{I}_{j}\). Figure 3 shows an example of such a decomposition. The space \(V^{I}_{0}\) is decomposed in \(V^{I}_{1}\) and \(W^{I}_{1}\), \(V^{I}_{1}\) in \(V^{I}_{2}\) and \(W^{I}_{2}\), and so on. Approximating a function in \(V^{I}_{0}\) is thus equivalent to approximating the same function in the boxed spaces and adding the solutions.
Let \(j_{\mathrm{max}}\) and \(j_{\mathrm{min}}\) denote the maximum and minimum scale used in the approximation, respectively. The approximation is then equivalent to one with scaling functions at scale \(j=j_{\mathrm{min}}1\). The basis for the adaptive resolution is
It contains all basis functions of \(V^{I}_{j_{\mathrm{max}}}\) (first set) to ensure that every point in the interval I is covered by at least one function. Moreover, it contains subsets of the bases of the spaces \(W^{I}_{j}\) for \(j=j_{\mathrm{min}},\dots ,j_{\mathrm{max}}\) (second set). The information which of the latter are used is stored in the \(\eta _{j}\)tuples \(\widehat{K}_{j}= (\widehat{K}_{j,1},\dots ,\widehat{K}_{j, \eta _{j}} )\). For these, \(\widehat{K}_{j,i}<\widehat{K}_{j,i'}\) for \(i< i'\) and \(1\leq \widehat{K}_{j,i}\leq \mathcal{D}_{j}\) for all i. How to choose the tuples is discussed later on page 10.
The tuples are also used to define the truncation matrices
where \(\mathbf{e}_{\widehat{K}_{j,n}}\in \mathbb{R}^{\mathcal{D}_{j}}\) is the \(\widehat{K}_{j,n}\)th unit column vector. The basis \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\) is used within a spectral method for the 1D heat equation from (2). This yields the semidiscrete equation
Herein, the used vectors and matrices as well as \(\mathbf{B}_{\mathrm{d}}\), the matrix used for the boundary conditions, are determined with the help of \(\mathbf{A}_{\mathrm{s}}\), \(\mathbf{M}_{\mathrm{s}}\), \(\mathbf{B}_{\mathrm{s}}\), \(\mathbf{u}_{\mathrm{s}}(t)\) and \(\mathbf{q}_{\mathrm{s}}(t)\). The subscript s stands for a static resolution, whereas d stands for a dynamic resolution. One would receive the static matrices and vectors if all wavelet basis functions in \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\) were used, i.e. with \(\widehat{K}_{j}= (1,\dots ,\mathcal{D}_{j} )\) for \(j=j_{\mathrm{min}},\dots ,j_{\mathrm{max}}\). Because of (11), these matrices and vectors can be derived from those from Sect. 3 at scale \(j_{\mathrm{min}}1\). With the transformation matrix
where \(\mathbf{I}_{\mathcal{D}_{j_{\mathrm{max}}}}\in \mathbb{R}^{ \mathcal{D}_{j_{\mathrm{max}}}\times \mathcal{D}_{j_{\mathrm{max}}}}\) is the identity matrix and \(\eta :=\mathcal{D}_{j_{\mathrm{max}}}+\sum_{j=j_{\mathrm{min}}}^{j_{ \mathrm{max}}}\eta _{j}\), one obtains
When changing the resolution, the matrices \(\mathbf{A}_{\mathrm{d}}\) and \(\mathbf{M}_{\mathrm{d}}\) have to be recalculated. Because \(\mathbf{A}_{\mathrm{s}}\) and \(\mathbf{M}_{\mathrm{s}}\) are known beforehand and \(\mathbf{T}^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\) is sparse, the computational costs for recalculation are low.
It remains to determine the tuples \(\widehat{K}_{j}\), where \(\langle \cdot ,\cdot \rangle := \vert (\cdot , \cdot ) \vert \) is used. Note that \(\langle \cdot ,\cdot \rangle \) is not an inner product but an abbreviation. The initial condition \(\theta _{0}(x)\) is used at the beginning of the simulation:
The basis function \(\hat{\psi }_{j,k}\) is used if the corresponding coefficient is greater than a tolerance \(\tau >0\), i.e. if the basis function \(\hat{\psi }_{j,k}\) has a significant contribution to the solution.
During the simulation it may occur that the resolution needs to be adapted. One has to distinguish between decreasing and increasing the resolution (see Fig. 4). For the former case, after every time step those basis functions whose coefficients are smaller than τ are removed from \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\). For the latter case, two different causes are considered. An increase of the resolution may be necessary due to the source term \(q(x,t)\) or heat flow. Because the source term is known beforehand, the required resolution can be determined as for the initial condition. The function \(\hat{\psi }_{j,k}\) is used if \(\langle q(x,t) ,\hat{\psi }_{j,k} \rangle >\tau \).
Because the solution of the PDE is approximated with the basis \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\), it is challenging to detect where a higher resolution caused by heat flow is needed. One possible approach is presented in the following.
Whenever a coefficient in \(\mathbf{u}_{\mathrm{d}}(t)\) changes from one time step to another by a certain factor α, the resolution in the interval of the support of the corresponding basis function \(\hat{\psi }_{j,k}\) is increased. Therefore, the wavelets at scale \(j1\), whose support is a subset of the support of \(\hat{\psi }_{j,k}\), are added to \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\), if \(j1\) does not exceed the minimum scale \(j_{\mathrm{min}}\), i.e. if \(j>j_{\mathrm{min}}\). Assuming that \(j>j_{\mathrm{min}}\), the scaling functions at scale \(j1\) with the indices
are added to \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\), i.e. \(\tilde{k}+1\in \widehat{K}_{j1}\) for all \(\tilde{k}\in \Lambda \). The corresponding coefficients to these wavelets are initialized with 0. Hence, the added wavelets must not be removed from \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\) for a time interval of length β because the coefficients may need a certain time to exceed the tolerance τ. This approach has been implemented and is used for the results in Sect. 7.3.
Adaptive quasi3D method
The ARM from the previous section is combined with a 2D FE method into an adaptive Q3D (AQ3D) method. The adaptivity only takes place in the longitudinal direction, i.e. the 2D mesh in the crosssection does not change. The method is derived for the 3D heat equation (6) and on the domain Ω defined in (7). The space for basis and test functions is
In contrast to the Q3D method, here the function g is chosen from the space \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\). With \(\{ \chi _{n}:n = 1,\dots ,\eta \} \) being a basis of \(\widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\), a basis for \(K^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\) is given by
with \(\nu _{m}\in S_{1}\) and \(\chi _{n}\in \widehat{\varXi }^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\).
Similar to (10), the semidiscrete equation is
Herein, the matrices can be written as
and
With (12) and (13) and the definition
where \(\mathbf{I}_{\mathcal{I}}\in \mathbb{R}^{\mathcal{I}\times \mathcal{I}}\) is the identity matrix, the matrices can be written as
and
The middle term is independent of the resolution and has to be calculated only once at the beginning of the simulation.
Similar to the matrices, the righthand side vector is
The boundary conditions are realized at \(S_{\mathrm{front}}\) and \(S_{\mathrm{back}}\) with the ARM and at \(S_{\mathrm{side}}\) with the FE method. The process of changing the resolution is very similar to the ARM. Here, a separate resolution is calculated for every edge in zdirection in the same way as explained in Sect. 5. The resolutions of all edges and the source term are then merged with each other to get a single resolution for all edges. Consequently, the matrix \(\mathbf{Q}^{j_{\mathrm{max}}}_{j_{\mathrm{min}}}\) can be recalculated and the simulation can proceed.
Simulation results
The time discretization for each method is realized with the implicit Euler method, where Δt denotes the step width. The difference between numerical and analytical solution is measured with
and
where \(t_{i}=i\Delta t\) is the time step. The norm \(\lVert \cdot \rVert _{\mathrm{max}}\) is used to compare θ̃ with an analytical solution as a function, whereas \(\lVert \cdot \rVert _{\infty }\) compares the vector u with a vector \(\mathbf{u}_{\mathrm{ana}}\) that contains the coefficients of the analytical solution.
Spectral scaling function method
For the spectral scaling function method (SSM), the 1D heat equation (2) with dimensionless \(L=10\), \(N=6\), \(\lambda =10\), \(c_{\mathrm{V}}=1\), \(\Delta t = 1 \cdot 10^{3}\) and 100 time steps is solved. The initial condition is \(\theta (x,0) = \sin (\frac{\pi }{L}x )\), the source term is \(q(x,t)=0\), and homogeneous Dirichlet boundary conditions are applied. The error between numerical and analytical solution is shown in Fig. 5. As expected, the error in both norms decreases with decreasing scale.
Quasi3D method
The Q3D method is used to simulate the temperature distribution for the benchmark problem defined in [8] and highlighted in red in Fig. 1. The domain consists of three insulated cables. They extend from \(z=0~\mbox{m}\) to \(z=1~\mbox{m}\) and are surrounded and separated by an insulation material (glass fiber). The problem’s spatial dimensions and material data are summarized in Tables 1 and 2, respectively. In the model, the cables have been homogenized into a bulk model consisting of one material, although in reality they are built up of several strands [21]. An initial condition of \(\theta _{0}(\mathbf{x}) = 2~\mbox{K}\) together with Dirichlet boundary conditions at the front (\(z=0~\mbox{m}\)) and back side (\(z=1~\mbox{m}\)) and homogeneous Neumann boundary conditions are applied at the hull. In order to simulate a quench in the left cable, the time independent source term
is applied, where \(\chi _{\mathrm{q}}(\mathbf{x})\) is equal to 1 in the left cable and equal to 0 elsewhere. The remaining values are chosen as \(q_{\mathrm{max}}=1 \cdot 10^{6}~\mathrm{W}\mbox{/}\mathrm{m}^{3}\), \(z_{\mathrm{q}}=0.33~\mbox{m}\) and \(\sigma =0.05~\mbox{m}\). For the simulation, scaling functions with \(N=6\) at scale −5 are used and 200 steps of the implicit Euler method with \(\Delta t=5\cdot 10^{5}~\mbox{s}\) are performed. This leads to a total simulation time of 10 ms.
In Fig. 6, the evolution of the temperature inside the three cables is shown. For this plot and for Fig. 7, the temperature was evaluated at \(z=z_{\mathrm{q}}\) and for each cable in the center of its crosssection. The temperature of the left cable increases immediately, while the other cables start to heat up after a certain time. At the end of the simulation (at \(t=10~\mbox{ms}\)) the left cable has thus the highest temperature. This can be seen in Fig. 7 and Fig. 8 as well. In Fig. 7 one can additionally see how the heat has already been flown from \(z=0.33~\mbox{m}\) in positive and negative zdirection. Figure 8 shows the temperature distribution at the end of the simulation at \(z=z_{\mathrm{q}}\) and displays the mesh in the crosssection. One can see that the temperature inside the three cables is nearly constant, whereas in the insulation material high temperature gradients are present. This temperature distribution is the result of the strongly differing values of the thermal conductivity of the cable and insulation (Table 2) and of the source term in (14), that is independent of x and y inside the left cable.
The Q3D method with scaling functions (denoted with Q3D_{sf}) is now compared to a Q3D_{poly} method (from [8]) and to a conventional 3D FE method. The Q3D_{poly} method uses a polynomial basis with a maximum degree M for the spectral method in longitudinal direction. It decomposes the longitudinal direction in nonequidistant intervals called elements. The problem that is solved can be found in (6) with dimensionless \(L=10\), \(\lambda =10\), \(c_{\mathrm{V}}=5\), \(\Delta t = 1 \cdot 10^{4}\) and 10 time steps. The initial condition is
and the source term is \(q(\mathbf{x},t)=0\). To the front and back side homogeneous Dirichlet boundary conditions and to the hull homogeneous Neumann boundary conditions are applied. With the chosen initial condition, the analytical solution of this problem is found by separation of variables as
The Q3D_{sf} method is used with \(N=6\) and the Q3D_{poly} method is used with a maximum polynomial degree \(M=4\) on each element in zdirection. The FE method uses a tetrahedral mesh with linear, nodal basis functions.
Figure 9 shows the error of the three methods with respect to the total number of basis functions. The error for the Q3D methods are measured in the maximum norm over all edges in zdirection and for the FE method the norm \(\lVert \cdot \rVert _{\infty }\) is used. The computed errors are comparable to each other. Both Q3D methods lead to significantly smaller errors than the FE method with a similar number of basis functions. Between the two Q3D methods there are no major differences. The errors of both methods are similar. However, the number of basis functions in longitudinal direction is more flexible in the Q3D_{poly} method because the polynomial degree and the number of elements can be chosen independently. For the Q3D_{sf} method in contrast, once N is set, only the scale can be varied what leads to a fixed number of basis functions.
Adaptive resolution method
The ARM is used to solve the 1D heat equation (2). The initial condition
and the boundary conditions \(\theta (0,t) = \theta _{0}(0)\ast H(0,t)\) and \(\theta (L,t) = \theta _{0}(L)\ast H(L,t)\), for \(t>0\), are used. Herein, \(H(x,t)\) is the fundamental solution of the 1D heat equation [22] and ∗ denotes convolution. Furthermore, \(L=10\), \(N=3\), \(\lambda =10\), \(c_{\mathrm{V}}=1\), \(\sigma = 0.15 \), \(\Delta t = 5 \cdot 10^{6}\). Moreover, 100 time steps are carried out and a tolerance \(\tau =1 \cdot 10^{8}\) is chosen.
In Fig. 10, the solution of the ARM is compared to those of the SSM. The error of the former method at a minimum scale \(j_{\mathrm{min}}\) has to be compared to the error of the latter at scale \(j=j_{\mathrm{min}}1\). Both methods yield the same error, as expected. However, the ARM uses less basis functions than the SSM. Figure 11 shows the number of used basis functions and the maximum possible number of basis functions for every time step and for the different minimum scale. As one can see, the actual number is below the maximum number of \(L2^{j_{\mathrm{min}}+1}\).
Adaptive Q3D method
For verification, the AQ3D method is used to solve the problem in (6) with dimensionless \(L=10\), \(\lambda =10\), \(c_{\mathrm{V}}=5\), \(\Delta t = 1\cdot 10^{4}\) and 10 time steps. The initial condition is taken from (15) and the source term is \(q(\mathbf{x},t)=0\). Homogeneous Dirichlet boundary conditions are applied on the front and back side, while homogeneous Neumann boundary conditions are applied to the hull. Figure 12 shows the maximum error between numerical and analytical solution over all edges in zdirection. The error on each edge is calculated with the infinity norm. The number of basis functions is increased by using both finer 2D meshes in the crosssection and a smaller minimum scale \(j_{\mathrm{min}}\) in longitudinal direction. Furthermore, the maximum scale is set to \(j_{\mathrm{max}}=1\) and for the spectral method, scaling functions and wavelets with \(N=6\) are utilized.
Lastly, to show the potential reduction of basis functions with the AQ3D method, it is used to solve the benchmark problem with three Rutherford cables defined in [8]. Instead of the cables being extended 1 m in zdirection, they are extended to 10 m for this simulation. Because the center of the source term is still \(z_{\mathrm{q}}=0.33~\mbox{m}\), there are no major differences expected in the temperature distribution between \(z=0~\mbox{m}\) and \(z=1~\mbox{m}\). The remaining parameters are the same as in Sect. 7.2. Moreover, scaling functions and wavelets with \(N=6\), \(j_{\mathrm{min}}=4\) and \(j_{\mathrm{max}}=3\) have been chosen. Thus, the results are comparable with the results from Sect. 7.2. The tolerance is \(\tau =1 \cdot 10^{4}\). With the indicated values, the maximum number of basis functions in longitudinal direction is 320. Furthermore, the used mesh in the cross section has 1289 nodes and 2496 elements. This leads to a maximum number of 412,480 basis functions for the AQ3D method.
In Fig. 13, the evolution of the temperature in the three cable is shown for the Q3D and the AQ3D method. Both methods lead to the same evolution. However, the number of basis functions of the AQ3D method is significantly lower than the maximum possible number of basis functions of 412,480 as depicted in Fig. 14. A simulation of this problem with the Q3D method with the same accuracy in the zdirection and the same mesh in the crosssection would require this maximum number of 412,480 basis functions.
Conclusion
A spectral method using Daubechies scaling functions has been formulated and verified. This has been combined with a 2D FE method with a nodal basis into a quasi3D method. With this method, a stack of three simplified Rutherford cables has been simulated successfully. A third method with an adaptive resolution in space and time has been formulated for the 1D heat equation. This method has been extended to a quasi3D method in the same manner as the spectral method. A comparison between the adaptive and associated nonadaptive methods showed a significant reduction of the number of basis functions, preserving the accuracy.
Availability of data and materials
Not applicable.
Abbreviations
 1D:

onedimensional
 2D:

twodimensional
 3D:

threedimensional
 AQ3D:

adaptive Q3D
 ARM:

Adaptive resolution method
 DBN :

DaubechiesN
 FE method:

Finite element method
 MRA:

Multiresolution analysis
 PDE:

Partial differential equation
 Q3D:

Quasi3D
 SSM:

Spectral scaling function method
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Acknowledgements
This work has been supported by the BMBF project “Quenchsimulation für Supraleitende Magnete: Steigerung der Auflösung in Zeit und Raum” (BMBF05P18RDRB1) and by the Graduate School Computational Engineering at TU Darmstadt. The research of Jonas Bundschuh is sponsored by the German Science Foundation (DFG project 436819664).
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The research and the numerical tests have been carried out by JB. JB and LAMD worked together on the manuscript. HDG acquired the funding and administrated the project. All authors have read and approved the final manuscript.
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Bundschuh, J., D’Angelo, L.A.M. & De Gersem, H. Quasi3D spectral wavelet method for a thermal quench simulation. J.Math.Industry 11, 17 (2021). https://doi.org/10.1186/s13362021001138
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DOI: https://doi.org/10.1186/s13362021001138
Keywords
 Finite element methods
 Hybrid discretizations
 Spectral element methods
 Wavelets
 Quenches