Numerical weather prediction (NWP) is a difficult task in chaotic dynamical regimes because of the strong sensitivity to initial conditions and physical parameters. As a result, high numerical accuracy is usually necessary. In this chapter, an accurate and efficient alternative to the traditional time stepping solution methods is presented; the time-spectral method. The generalized weighted residual method (GWRM) solves systems of nonlinear ODEs and PDEs using a spectral representation of time. Not being subject to CFL-like criteria, the GWRM typically employs time intervals two orders of magnitude larger than those of time-stepping methods. As an example, efficient solution of the chaotic Lorenz 1984 equations is demonstrated. The results indicate that the method has strong potential for NWP. Furthermore, employing spectral representations of physical parameters and initial values, families of solutions are obtained in a single computation. Thus, the GWRM is conveniently used for studies of system parameter dependency and initial condition error growth in NWP.
- error analysis
- initial condition
Numerical methods are routinely used when modeling complex systems such as meteorological and atmospheric systems. These systems can be described by nonlinear ordinary and partial differential equations. Nonlinear systems in particular, as opposed to linear systems, constitute specific numerical challenges in terms of processing and memory requirements. In order to efficiently use the computer’s resources, it is important to choose a suitable numerical method .
Typically, when solving initial value ODEs, it is common practice to use finite difference methods (FDM) that discretize the temporal domain into finite steps. Information from the initial state and previously computed steps are used to estimate the solution at a “future” discrete time step. This is an intuitive and powerful method because we can easily visualize the cause and effect of each step. However, the problem with these techniques when solving complex systems is that small temporal steps are required in order for a solution to be found. In order to acquire a stable solution, the Courant-Friedrichs-Lewy (CFL) condition needs to be satisfied when employing more accurate, explicit FDM, thus limiting time step length.
Another approach is to use a time-spectral method, which takes a bird’s eye view of the problem [2, 3, 4, 5, 6, 7]. Instead of focusing on small local steps in time, an approximate solution that could fit the entire temporal domain is postulated. This approximate solution is set in the form of a finite series of basis functions. Thus, the unknowns of the equations are thereby changed from the physical variables to the coefficients of the solution ansatz. The procedure allows for highly accurate and global temporal solutions.
In the following, we will present application of the GWRM  to the Lorenz 1984  differential equations. This is a set of three coupled, nonlinear, and chaotic ODEs, providing a basic model of the important process of Hadley tropical atmospheric circulation. In Section 2, Method, we present a short derivation of the GWRM. Section 3 will introduce the Lorenz equations and how they can be solved by the time-spectral method. In this section, we also show how the parameter dependence of the solution can be found from a
The time-spectral method employed here is the generalized weighted residual method (GWRM). The physical equations of this Galerkin method are projected onto a space of weighted orthogonal basis functions resulting in a set of algebraic equations. The residual of the differential equation is necessarily zero for the exact solution, thus the numerical method seeks to solve for the coefficients that minimize the residual in the interval where orthogonality holds.
In this procedure, all dimensions can be included, thus the term “generalized.” This means that the dependence on all
A key characteristic of Chebyshev polynomials, and a main reason for choosing them as basis functions, is their
2.1. Generalized weighted residual method
Consider the following set of differential equations,
where is the unknown variable with a temporal, spatial, and parameter dependence. is a linear or nonlinear operator, and is a source term. The GWRM solution ansatz takes the form, in the case of a singular physical dimension and one parameter,
Here, is the Chebyshev polynomial of the first kind, are coefficients, and the prime () denotes that the first term of each summation should be multiplied by . Since Chebyshev polynomials are orthogonal in the interval , variable transformations are applied for general intervals,
where and , being the variable , , and with their respective upper and lower bounds. The Picard integral is then applied to (1), after which the residual of the differential equation is formed,
The residual is multiplied by weighted Chebyshev polynomials and then integrated over the computational domain, whereafter it is set to zero. The equation takes the form
where the Chebyshev weight is , being the transform variables , , and . Eq. (5) has the form of an
Continuing, we expand Eq. (5),
yielding the following relations for each term of (6):
where are the solution coefficients, is the Kronecker delta function, represents the initial conditions, is the spectral representation of the time-integrated linear or nonlinear operator , and represents the time-integrated source term. Eq. (10) is here defined for the truncated domain , whereas strictly the time integration renders terms. For the spatial domain, we have , where , with representing the total number of boundary conditions for this spatial dimension. Boundary condition equations are thus added to (10) for problems including spatial derivatives. Here, we will be solving a set of time-dependent ODEs, thus only initial conditions are required to find a unique solution. Finally, it holds that .
Eq. (10) can be solved iteratively with a suitable root solver. Here, we use the semi-implicit root solver (SIR)  because it shows superior global stability compared to the Newton method (NM) with line-search while still maintaining a fast convergence.
3. The GWRM, exemplified by the Lorenz 1984 equations
The Lorenz 1984 model is a set of three nonlinear ordinary differential equations that features chaotic behavior similar to that of meteorological systems . It is consequently one of the simplest models of Hadley circulation due to the substantial amount of approximations postulated in order to arrive at this low order model. Thus, whereas the Lorenz 1984 model is not an accurate NWP model, it allows for a rigorous numerical analysis of simple, yet nonlinear chaotic behavior. This is the reason for employing them in the present work. The equations are
For a more exhaustive description of the model, see . Suffice it to say the variables , , and represent certain meteorological systems such as wind currents and large-scale eddies. The coefficients , , , and are chosen within certain limits to act as damping, coupling, and amplification of the physical processes of the system.
Lorenz, in his 1984 article, posed the question, “What can such a simple model possibly tell us about the real atmosphere?”. His answer was that postulating certain hypothesis about the behavior of the real atmosphere, we can strengthen the reasoning behind the hypothesis qualitatively by the help of these models. However, that is not what we are concerned with here, but rather the model is used as a test to show how different numerical methods handle chaotic behavior. Furthermore, the model is useful to develop new techniques that can analyze such quantities as error growth, parameter uncertainties, and variable perturbations in a more efficient way.
3.1. Time intervals
The GWRM is a global method where a finite number of Chebyshev modes are used to represent the physics in a given temporal domain. Instead of using a large number of Chebyshev modes to obtain a single solution for the entire temporal domain, it is more efficient to split the domain into smaller subintervals, so that lesser Chebyshev modes can be used in each interval.
For controlling and maintaining the same numerical accuracy within each time interval, an automatic
where , , are the Chebyshev coefficients with as the highest mode. By requiring that , where is a stipulated accuracy, the time subintervals to achieve this accuracy are automatically computed. We have found it efficient to use a balanced algorithm that tries to expand the time interval at about every 10th time interval by a factor 1.5, and that halves the interval whenever accuracy could not be achieved.
An interesting and useful property of Chebyshev polynomials is , so that
Thus, the exact solution at the end state can be approximated by a sum of the Chebyshev coefficients. Eq. (13) conveniently allows for the previous end conditions, represented as Chebyshev coefficients, to be applied as initial conditions for the next interval. All computations of a series of connected intervals are thus calculated in
The pseudocode shows the following: the algebraic equations are collected in a vector , along with the initial conditions in the first element of the vector. The time domain is divided into subintervals in which the equations are solved by SIR. The initial condition is equal to the end-state of the previous solution, see (13). If the convergence parameter “
3.2. Parameter dependency
Instruments are continually measuring the weather’s temperature, wind speeds, and topological height and width to name a few parameters. However, the measurement devices cannot, at present, give a global coverage. Thus, meteorological parameters are approximate and interpolated.
The meteorological parameters are represented in the Lorenz model by , , , and . The uncertainty of the measured parameters will inevitably lower the confidence of the solution, specifically important in weather prediction.
When studying parameter dependencies, the GWRM enables an interesting solution. Instead of assigning the parameter a single value, we can introduce a
For the Lorenz ODEs, where we have temporal and parameter dependencies, the solution ansatz then takes the form,
In Eq. (14), a single parameter has been included; however, the procedure can be expanded to any number of parameters. The impact of the parameter from the Lorenz equation (11) on the variable is demonstrated in Figure 1. The result from a single GWRM computation is displayed, using the ansatz (14). It can be seen that varying with the other parameters of Eq. (11) held fixed, the solution is strongly dependent on for longer times. For lower values of , the solution becomes more stable and fluctuates with a higher frequency than for higher values of .
It is of interest to provide a quantitative measure of the effect of on the solution. One approach would be to compare the deviations from a “base” run for different values of . For simplicity, however, we have chosen to monitor the standard deviations as a measure of the deflection from the average value in the entire parameter interval. Standard deviations can be computed from the semianalytical solutions with the formula
where is the GWRM solution for a specific value of the parameter. The evaluations have been carried out at parameter points at a time of interest. The parameter interval averaged solution is denoted by . A table is presented below where comparisons are made with a base run with specified parameter values , , , and . The solution at is used. Average values and standard deviations , representing the entire parameter interval are also given.
The standard deviations are supplied with indices to indicate the chosen parameter and variable for analysis. For example, states that is the parameter domain and the standard deviation of is being analyzed. One parameter at a time has been varied by , while the others are kept constant.
|Parameter dependency example, using a single GWRM computation , ,|
It is immediately seen that the variable is strongly affected by changes in all parameter values, whereas the and solutions are more robust.
3.3. Initial condition uncertainty
Meteorological models generally include time-dependent PDEs and ODEs that require initial conditions as starting points. In mathematical terms, initial conditions are required to close the system of equations. If we are interested in computing a family of scenarios employing different initial conditions, the standard approach to determine the final states is to restart the computations from scratch, using a new initial condition each time.
Time-spectral methods offer a more convenient approach. Similarly, as when we computed parameter dependency in a single GWRM computation in the previous section, we will now study the effect of a spectrum of initial values on the solution of Eq. (11), employing a single GWRM computation.
|Initial condition dependency example, using a single GWRM computation , ,|
An interesting, albeit challenging, feature of meteorological models is the
A classical error growth analysis employed for the Lorenz equations (11) would be the following. A base scenario (where denotes the variable) with initial conditions with a time window of is solved for. Subsequently, a number of perturbed scenarios are solved, denoted with superscript , where the initial conditions are perturbed an amount , taking values , for example. The error growth is then computed with the formula,
Thus, in this traditional analysis, a large number of computations are needed, where the ODEs are solved for different perturbed initial conditions.
We suggest another approach. By use of an ansatz of the type (14), a spectrum of initial conditions is allowed in a single computation. In the table above, results are presented for three cases where Eq. (11) has been solved to time . For the three cases, the base initial conditions , , and as well as intervals for , , and are shown. Also, results for the base initial conditions at are provided. For the solutions, where the initial conditions are allowed to vary in an interval, both averages over the interval are shown as well as corresponding standard deviations. The analysis shows that the variable value at is strongly dependent on the initial condition. In Figure 2, the time and initial condition dependence of the variable is shown in a 3D diagram. Here, the run time has been extended to .
It would also be of interest to study the effect of allowing the initial conditions for all variables , , and to vary simultaneously. In order to accomplish this in a single GWRM run, the natural thing to do would be to extend the ansatz (14) to include three parameters, corresponding to the different initial conditions. Instead, we have chosen a simpler approach. We let , , and , where the perturbation is a single parameter that is applied to all three variables. An example computation is shown in Figure 3. The variable here features a quite a different time evolution than in Figure 2, where only the variable initial condition was perturbed.
In the table below, initial condition interval average values, as well as standard deviations, are provided for all the variables , , and for a run extending to .
|Initial condition dependency example, using a single GWRM computation , , ,|
Returning to error growth analysis as suggested by Eq. (16), reliable results can be computed if a sufficiently large domain has been spanned by the perturbed initial conditions. We have compared the classical approach of perturbed iterations (PI) with the new initial condition parameter dependency (ICPD) technique in Figure 4a and b. Of particular interest is the potential gain in CPU time, using the ICPD.
It is found that the ICPD technique with and achieves the same result of error growth as the PI scheme. The ICPD scheme computed the error growth in as compared to the PI scheme which required . Thus, a near fivefold increase in efficiency was obtained for this relatively simple case.
Is it more
the parameter dependencies can easily be analyzed since GWRM solutions are analytical
the time-spectral method is a high-order method, leading to high accuracy solutions
all parameters in an interval are included, whereas certain regions of critical parameter dependence could be missed out with traditional PI methods
the parameter domain can be split into intervals, that can be solved for separately, potentially spanning a larger parameter space more efficiently
In this chapter, a univariate analysis has been performed; however, a multivariate analysis can also be implemented in the same manor. It should be noted, however, that the more parameters introduced in the analysis, the more Chebyshev modes need to be solved for, which results in larger matrices and memory demands.
It is also of interest to address the
Spectral methods have a long history when applied to the spatial domain in PDE modeling. The time-spectral method GWRM, demonstrated here, provides similar accuracy for the temporal domain. High-order methods, like the GWRM, may achieve resolutions much higher than that of finite difference methods for similar amount of work. Furthermore, when applied to meteorological systems, the time-spectral method can accurately and efficiently compute the physics in all spatial, temporal, and parameter domains.
A recent study, comparing the time-spectral method GWRM with commonly used time-stepping methods such as Runge-Kutta and other, high-order implicit methods, was carried out in . Since then, the GWRM numerical algorithms have been further streamlined; see for example . Moreover, it has been found that the Jacobian of the algebraic system of equations (10) need only be computed once by including the time interval length analytically. Thus, during the computations, the new time interval length can be substituted into the Jacobian before use. This decreases the computation time from to , roughly , for perturbed scenarios with and .
We have, in this chapter, also presented a new approach to error analysis using the initial condition parameter dependency (ICPD) technique, that is, by spectral representation of the parameter domain. In a single computation, the same error growth was reproduced as for the classical case (where a large number of runs were carried out for different initial conditions), with a computational time of . This amounts to a near fivefold gain in CPU time efficiency.
Finally, it was shown that the ICPD technique is also successfully applicable for determining the effect of perturbed physical variables on the solution. In one GWRM computation only, it was found that the solutions to the Lorenz 1984 equations sensitively depend on the system parameter .
|Algorithm 1. GWRM time Intervals.|