.. include:: links.inc .. _sec-tutorial: Tutorial ======== .. only:: html .. contents:: Table of Contents :local: :backlinks: top Basic *SfePy* Usage ------------------- *SfePy* package can be used in two basic ways as a: #. Black-box Partial Differential Equation (PDE) solver, #. Python package to build custom applications involving solving PDEs by the Finite Element Method (FEM). This tutorial focuses on the first way and introduces the basic concepts and nomenclature used in the following parts of the documentation. Check also the :doc:primer which focuses on a particular problem in detail. Users not familiar with the finite element method should start with the :ref:sec-solving-pdes-fem. .. _invoking_from_command_line: Invoking *SfePy* from the Command Line ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ This section introduces the basics of running *SfePy* from the command line, assuming it was properly installed, see :ref:introduction_installation. The command sfepy-run is the **most basic starting point** in *SfePy*. It can be used to run declarative problem description files (see below) as follows:: sfepy-run Using *SfePy* Interactively ^^^^^^^^^^^^^^^^^^^^^^^^^^^ All functions of *SfePy* package can be also used interactively (see :ref:sec-interactive-example-linear-elasticity for instance). We recommend to use the IPython_ interactive shell for the best fluent user experience. You can customize your IPython startup profile as described in :ref:using-ipython. Basic Notions ------------- The simplest way of using *SfePy* is to solve a system of PDEs defined in a problem description file, also referred to as input file. In such a file, the problem is described using several keywords that allow one to define the equations, variables, finite element approximations, solvers and solution domain and subdomains (see :ref:sec-problem-description-file for a full list of those keywords). The syntax of the problem description file is very simple yet powerful, as the file itself is just a regular Python module that can be normally imported -- no special parsing is necessary. The keywords mentioned above are regular Python variables (usually of the dict type) with special names. Below we show: * how to solve a problem given by a problem description file, and * explain the elements of the file on several examples. But let us begin with a slight detour... Sneak Peek: What is Going on Under the Hood ^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^ #. A command (usually sfepy-run as in this tutorial) or a script reads in an input file. #. Following the contents of the input file, a Problem instance is created -- this is the input file coming to life. Let us call the instance problem. * The Problem instance sets up its domain, regions (various sub-domains), fields (the FE approximations), the equations and the solvers. The equations determine the materials and variables in use -- only those are fully instantiated, so the input file can safely contain definitions of items that are not used actually. #. The solution is then obtained by calling problem.solve() function, which in turn calls a top-level time-stepping solver. In each step, problem.time_update() is called to setup boundary conditions, material parameters and other potentially time-dependent data. The problem.save_state() is called at the end of each time step to save the results. This holds also for stationary problems with a single "time step". So that is it -- using the code a black-box PDE solver shields the user from having to create the Problem instance by hand. But note that this is possible, and often necessary when the flexibility of the default solvers is not enough. At the end of the tutorial an example demonstrating the interactive creation of the Problem instance is shown, see :ref:sec-interactive-example-linear-elasticity. Now let us continue with running a simulation. Running a Simulation -------------------- The following commands should be run in the top-level directory of the *SfePy* source tree after compiling the C extension files. See :ref:introduction_installation for full installation instructions. * Download :download:sfepy/examples/diffusion/poisson_short_syntax.py <../sfepy/examples/diffusion/poisson_short_syntax.py>. It represents our sample *SfePy* :ref:sec-problem-description-file, which defines the problem to be solved in terms *SfePy* can understand. * Use the downloaded file in place of  and run sfepy-run as :ref:described above . The successful execution of the command creates output file cylinder.vtk in the *SfePy* top-level directory. .. _postprocessing: Postprocessing the Results ^^^^^^^^^^^^^^^^^^^^^^^^^^ * The sfepy-view command can be used for quick postprocessing and visualization of the *SfePy* output files. It requires pyvista_ installed on your system. * As a simple example, try:: sfepy-view cylinder.vtk * The following interactive 3D window should display: .. image:: images/resview/resview_shot3.png :width: 70 % :align: center * You can manipulate displayed image using: * the left mouse button by itself orbits the 3D view, * holding shift and the left mouse button pans the view, * holding control and the left mouse button rotates about the screen normal axis, * the right mouse button controls the zoom. .. _poisson-example-tutorial: Example Problem Description File -------------------------------- Here we discuss the contents of the :download:sfepy/examples/diffusion/poisson_short_syntax.py <../sfepy/examples/diffusion/poisson_short_syntax.py> problem description file. For additional examples, see the problem description files in the sfepy/examples/ directory of *SfePy*. The problem at hand is the following: .. math:: :label: eq_laplace_static c \Delta T = f \mbox{ in }\Omega,\quad T(t) = \bar{T}(t) \mbox{ on } \Gamma \;, where :math:\Gamma \subseteq \Omega is a subset of the domain :math:\Omega boundary. For simplicity, we set :math:f \equiv 0, but we still work with the material constant :math:c even though it has no influence on the solution in this case. We also assume zero fluxes over :math:\partial \Omega \setminus \Gamma, i.e. :math:\pdiff{T}{\ul{n}} = 0 there. The particular boundary conditions used below are :math:T = 2 on the left side of the cylindrical domain depicted in the previous section and :math:T = -2 on the right side. The first step to do is to write :eq:eq_laplace_static in *weak formulation* :eq:eq_wpoisson_final. The :math:f = 0, :math:g = \pdiff{T}{\ul{n}} = 0. So only one term in weak form :eq:eq_wpoisson_final remains: .. math:: :label: eq_wlaplace_static \int_{\Omega} c\ \nabla T \cdot \nabla s = 0, \quad \forall s \in V_0 \;. Comparing the above integral term with the long table in :ref:term_overview, we can see that *SfePy* contains this term under name dw_laplace. We are now ready to proceed to the actual problem definition. Open the :download:sfepy/examples/diffusion/poisson_short_syntax.py <../sfepy/examples/diffusion/poisson_short_syntax.py> file in your favorite text editor. Note that the file is a regular Python source code. :: from sfepy import data_dir filename_mesh = data_dir + '/meshes/3d/cylinder.mesh' The filename_mesh variable points to the file containing the mesh for the particular problem. *SfePy* supports a variety of mesh formats. :: materials = { 'coef': ({'val' : 1.0},), } Here we define just a constant coefficient :math:c of the Poisson equation, using the 'values' attribute. Other possible attribute is 'function' for material coefficients computed/obtained at runtime. Many finite element problems require the definition of material parameters. These can be handled in *SfePy* with material variables which associate the material parameters with the corresponding region of the mesh. :: regions = { 'Omega' : 'all', # or 'cells of group 6' 'Gamma_Left' : ('vertices in (x < 0.00001)', 'facet'), 'Gamma_Right' : ('vertices in (x > 0.099999)', 'facet'), } Regions assign names to various parts of the finite element mesh. The region names can later be referred to, for example when specifying portions of the mesh to apply boundary conditions to. Regions can be specified in a variety of ways, including by element or by node. Here, 'Omega' is the elemental domain over which the PDE is solved and 'Gamma_Left' and 'Gamma_Right' define surfaces upon which the boundary conditions will be applied. :: fields = { 'temperature': ('real', 1, 'Omega', 1) } A field is used mainly to define the approximation on a (sub)domain, i.e. to define the discrete spaces :math:V_h, where we seek the solution. The Poisson equation can be used to compute e.g. a temperature distribution, so let us call our field 'temperature'. On the region 'Omega' it will be approximated using linear finite elements. A field in a given region defines the finite element approximation. Several variables can use the same field, see below. :: variables = { 't': ('unknown field', 'temperature', 0), 's': ('test field', 'temperature', 't'), } One field can be used to generate discrete degrees of freedom (DOFs) of several variables. Here the unknown variable (the temperature) is called 't', it's associated DOF name is 't.0' -- this will be referred to in the Dirichlet boundary section (ebc). The corresponding test variable of the weak formulation is called 's'. Notice that the 'dual' item of a test variable must specify the unknown it corresponds to. For each unknown (or state) variable there has to be a test (or virtual) variable defined, as usual in weak formulation of PDEs. :: ebcs = { 't1': ('Gamma_Left', {'t.0' : 2.0}), 't2', ('Gamma_Right', {'t.0' : -2.0}), } Essential (Dirichlet) boundary conditions can be specified as above. Boundary conditions place restrictions on the finite element formulation and create a unique solution to the problem. Here, we specify that a temperature of +2 is applied to the left surface of the mesh and a temperature of -2 is applied to the right surface. :: integrals = { 'i': 2, } Integrals specify which numerical scheme to use. Here we are using a 2nd order quadrature over a 3 dimensional space. :: equations = { 'Temperature' : """dw_laplace.i.Omega( coef.val, s, t ) = 0""" } The equation above directly corresponds to the discrete version of :eq:eq_wlaplace_static, namely: Find :math:\bm{t} \in V_h, such that .. math:: \bm{s}^T (\int_{\Omega_h} c\ \bm{G}^T G) \bm{t} = 0, \quad \forall \bm{s} \in V_{h0} \;, where :math:\nabla u \approx \bm{G} \bm{u}. The equations block is the heart of the *SfePy* problem description file. Here, we are specifying that the Laplacian of the temperature (in the weak formulation) is 0, where coef.val is a material constant. We are using the 'i' integral defined previously, over the domain specified by the region 'Omega'. The above syntax is useful for defining *custom integrals* with user-defined quadrature points and weights, see :ref:ug_integrals. The above uniform integration can be more easily achieved by:: equations = { 'Temperature' : """dw_laplace.2.Omega( coef.val, s, t ) = 0""" } The integration order is specified directly in place of the integral name. The integral definition is superfluous in this case. :: solvers = { 'ls' : ('ls.scipy_direct', {}), 'newton' : ('nls.newton', {'i_max' : 1, 'eps_a' : 1e-10, }), } Here, we specify the linear and nonlinear solver kinds and options. See :mod:sfepy.solvers.ls, :mod:sfepy.solvers.nls and :mod:sfepy.solvers.ts_solvers for available solvers and their parameters.. Even linear problems are solved by a nonlinear solver (KISS rule) -- only one iteration is needed and the final residual is obtained for free. Note that we do not need to define a time-stepping solver here - the problem is stationary and the default 'ts.stationary' solver is created automatically. :: options = { 'nls' : 'newton', 'ls' : 'ls', } The solvers to use are specified in the options block. We can define multiple solvers with different convergence parameters. That's it! Now it is possible to proceed as described in :ref:invoking_from_command_line. .. _sec-interactive-example-linear-elasticity: Interactive Example: Linear Elasticity -------------------------------------- This example shows how to use *SfePy* interactively, but also how to make a custom simulation script. We will use IPython_ interactive shell which allows more flexible and intuitive work (but you can use standard Python shell as well). We wish to solve the following linear elasticity problem: .. math:: :label: eq_linear_elasticity - \pdiff{\sigma_{ij}(\ul{u})}{x_j} + f_i = 0 \mbox{ in }\Omega, \quad \ul{u} = 0 \mbox{ on } \Gamma_1, \quad u_1 = \bar{u}_1 \mbox{ on } \Gamma_2 \;, where the stress is defined as :math:\sigma_{ij} = 2 \mu e_{ij} + \lambda e_{kk} \delta_{ij}, :math:\lambda, :math:\mu are the LamÃ©'s constants, the strain is :math:e_{ij}(\ul{u}) = \frac{1}{2}(\pdiff{u_i}{x_j} + \pdiff{u_j}{x_i}) and :math:\ul{f} are volume forces. This can be written in general form as :math:\sigma_{ij}(\ul{u}) = D_{ijkl} e_{kl}(\ul{u}), where in our case :math:D_{ijkl} = \mu (\delta_{ik} \delta_{jl}+\delta_{il} \delta_{jk}) + \lambda \ \delta_{ij} \delta_{kl}. In the weak form the equation :eq:eq_linear_elasticity is .. math:: :label: eq_wlinear_elasticity \int_{\Omega} D_{ijkl} e_{kl}(\ul{u}) e_{ij}(\ul{v}) + \int_{\Omega} f_i v_i = 0 \;, where :math:\ul{v} is the test function, and both :math:\ul{u}, :math:\ul{v} belong to a suitable function space. **Hint:** Whenever you create a new object (e.g. a Mesh instance, see below), try to print it using the print statement -- it will give you insight about the object internals. The whole example summarized in a script is available below in :ref:tutorial_interactive_source. In the *SfePy* top-level directory run :: ipython .. sourcecode:: ipython In [1]: import numpy as nm In [2]: from sfepy.discrete.fem import Mesh, FEDomain, Field Read a finite element mesh, that defines the domain :math:\Omega. .. sourcecode:: ipython In [3]: mesh = Mesh.from_file('meshes/2d/rectangle_tri.mesh') Create a domain. The domain allows defining regions or subdomains. .. sourcecode:: ipython In [4]: domain = FEDomain('domain', mesh) Define the regions -- the whole domain :math:\Omega, where the solution is sought, and :math:\Gamma_1, :math:\Gamma_2, where the boundary conditions will be applied. As the domain is rectangular, we first get a bounding box to get correct bounds for selecting the boundary edges. .. sourcecode:: ipython In [5]: min_x, max_x = domain.get_mesh_bounding_box()[:, 0] In [6]: eps = 1e-8 * (max_x - min_x) In [7]: omega = domain.create_region('Omega', 'all') In [8]: gamma1 = domain.create_region('Gamma1', ...: 'vertices in x < %.10f' % (min_x + eps), ...: 'facet') In [9]: gamma2 = domain.create_region('Gamma2', ...: 'vertices in x > %.10f' % (max_x - eps), ...: 'facet') Next we define the actual finite element approximation using the :class:Field  class. .. sourcecode:: ipython In [10]: field = Field.from_args('fu', nm.float64, 'vector', omega, ....: approx_order=2) Using the field fu, we can define both the unknown variable :math:\ub and the test variable :math:\vb. .. sourcecode:: ipython In [11]: from sfepy.discrete import (FieldVariable, Material, Integral, Function, ....: Equation, Equations, Problem) In [12]: u = FieldVariable('u', 'unknown', field) In [13]: v = FieldVariable('v', 'test', field, primary_var_name='u') Before we can define the terms to build the equation of linear elasticity, we have to create also the materials, i.e. define the (constitutive) parameters. The linear elastic material m will be defined using the two LamÃ© constants :math:\lambda = 1, :math:\mu = 1. The volume forces will be defined also as a material as a constant (column) vector :math:[0.02, 0.01]^T. .. sourcecode:: ipython In [14]: from sfepy.mechanics.matcoefs import stiffness_from_lame In [15]: m = Material('m', D=stiffness_from_lame(dim=2, lam=1.0, mu=1.0)) In [16]: f = Material('f', val=[[0.02], [0.01]]) One more thing needs to be defined -- the numerical quadrature that will be used to integrate each term over its domain. .. sourcecode:: ipython In [17]: integral = Integral('i', order=3) Now we are ready to define the two terms and build the equations. .. sourcecode:: ipython In [18]: from sfepy.terms import Term In [19]: t1 = Term.new('dw_lin_elastic(m.D, v, u)', ....: integral, omega, m=m, v=v, u=u) In [20]: t2 = Term.new('dw_volume_lvf(f.val, v)', ....: integral, omega, f=f, v=v) In [21]: eq = Equation('balance', t1 + t2) In [22]: eqs = Equations([eq]) The equations have to be completed by boundary conditions. Let us clamp the left edge :math:\Gamma_1, and shift the right edge :math:\Gamma_2 in the :math:x direction a bit, depending on the :math:y coordinate. .. sourcecode:: ipython In [23]: from sfepy.discrete.conditions import Conditions, EssentialBC In [24]: fix_u = EssentialBC('fix_u', gamma1, {'u.all' : 0.0}) In [25]: def shift_u_fun(ts, coors, bc=None, problem=None, shift=0.0): ....: val = shift * coors[:,1]**2 ....: return val In [26]: bc_fun = Function('shift_u_fun', shift_u_fun, ....: extra_args={'shift' : 0.01}) In [27]: shift_u = EssentialBC('shift_u', gamma2, {'u.0' : bc_fun}) The last thing to define before building the problem are the solvers. Here we just use a sparse direct *SciPy solver* and the *SfePy Newton solver* with default parameters. We also wish to store the convergence statistics of the Newton solver. As the problem is linear it should converge in one iteration. .. sourcecode:: ipython In [28]: from sfepy.base.base import IndexedStruct In [29]: from sfepy.solvers.ls import ScipyDirect In [30]: from sfepy.solvers.nls import Newton In [31]: ls = ScipyDirect({}) In [32]: nls_status = IndexedStruct() In [33]: nls = Newton({}, lin_solver=ls, status=nls_status) Now we are ready to create a Problem instance. .. sourcecode:: ipython In [34]: pb = Problem('elasticity', equations=eqs) The :class:Problem  has several handy methods for debugging. Let us try saving the regions into a VTK file. .. sourcecode:: ipython In [35]: pb.save_regions_as_groups('regions') And view them :: In [36]: ! sfepy-view regions.vtk -2 --grid-vector1 "[2, 0, 0]" You should see this: .. image:: images/linear_elasticity_regions.png :width: 80 % :align: center Finally, we set the boundary conditions and the top-level solver , solve the problem, save and view the results. For stationary problems, the top-level solver needs not to be a time-stepping solver - when a nonlinear solver is set instead, the default 'ts.stationary' time-stepping solver is created automatically. .. sourcecode:: ipython In [39]: pb.set_bcs(ebcs=Conditions([fix_u, shift_u])) In [40]: pb.set_solver(nls) In [41]: status = IndexedStruct() In [42]: variables = pb.solve(status=status) In [43]: print('Nonlinear solver status:\n', nls_status) In [44]: print('Stationary solver status:\n', status) In [45]: pb.save_state('linear_elasticity.vtk', variables) This :: sfepy-view linear_elasticity.vtk -2 is used to produce the resulting image: .. image:: images/linear_elasticity_solution1.png :width: 80 % :align: center The default view is not very fancy. Let us show the displacements by shifting the mesh. Close the previous window and do :: sfepy-view linear_elasticity.vtk -2 -f u:wu:p0 1:vw:p0 And the result is: .. image:: images/linear_elasticity_solution2.png :width: 80 % :align: center .. _tutorial_interactive_source: Complete Example as a Script ^^^^^^^^^^^^^^^^^^^^^^^^^^^^ The source code: :download:linear_elastic_interactive.py <../sfepy/examples/linear_elasticity/linear_elastic_interactive.py>. This file should be run from the top-level *SfePy* source directory so it can find the mesh file correctly. Please note that the provided example script may differ from above tutorial in some minor details. .. literalinclude:: ../sfepy/examples/linear_elasticity/linear_elastic_interactive.py :linenos: