コード例 #1
0
ファイル: CoupledRK3.py プロジェクト: rmatsumiya/spectralDNS
def get_context():
    """Set up context for solver"""

    collapse_fourier = False if params.dealias == '3/2-rule' else True
    family = 'C'
    ST = FunctionSpace(params.N[0], family, bc=(0, 0), quad=params.Dquad)
    CT = FunctionSpace(params.N[0], family, quad=params.Dquad)
    CP = FunctionSpace(params.N[0], family, quad=params.Dquad)
    K0 = FunctionSpace(params.N[1], 'F', domain=(0, params.L[1]), dtype='D')
    K1 = FunctionSpace(params.N[2], 'F', domain=(0, params.L[2]), dtype='d')
    #CP.slice = lambda: slice(0, CP.N-2)

    constraints = ((3, 0, 0), (3, params.N[0] - 1, 0))

    kw0 = {
        'threads': params.threads,
        'planner_effort': params.planner_effort["dct"],
        'slab': (params.decomposition == 'slab'),
        'collapse_fourier': collapse_fourier
    }
    FST = TensorProductSpace(comm, (ST, K0, K1), **kw0)  # Dirichlet
    FCT = TensorProductSpace(comm, (CT, K0, K1), **kw0)  # Regular Chebyshev N
    FCP = TensorProductSpace(comm, (CP, K0, K1),
                             **kw0)  # Regular Chebyshev N-2
    VFS = VectorSpace(FST)
    VCT = VectorSpace(FCT)
    VQ = CompositeSpace([VFS, FCP])

    mask = FST.get_mask_nyquist() if params.mask_nyquist else None

    # Padded
    kw = {
        'padding_factor': 1.5 if params.dealias == '3/2-rule' else 1,
        'dealias_direct': params.dealias == '2/3-rule'
    }
    if params.dealias == '3/2-rule':
        # Requires new bases due to planning and transforms on different size arrays
        STp = FunctionSpace(params.N[0], family, bc=(0, 0), quad=params.Dquad)
        CTp = FunctionSpace(params.N[0], family, quad=params.Dquad)
    else:
        STp, CTp = ST, CT
    K0p = FunctionSpace(params.N[1],
                        'F',
                        dtype='D',
                        domain=(0, params.L[1]),
                        **kw)
    K1p = FunctionSpace(params.N[2],
                        'F',
                        dtype='d',
                        domain=(0, params.L[2]),
                        **kw)
    FSTp = TensorProductSpace(comm, (STp, K0p, K1p), **kw0)
    FCTp = TensorProductSpace(comm, (CTp, K0p, K1p), **kw0)
    VFSp = VectorSpace(FSTp)
    VCp = CompositeSpace([FSTp, FCTp, FCTp])

    float, complex, mpitype = datatypes("double")

    # Mesh variables
    X = FST.local_mesh(True)
    x0, x1, x2 = FST.mesh()
    K = FST.local_wavenumbers(scaled=True)

    # Solution variables
    UP_hat = Function(VQ)
    UP_hat0 = Function(VQ)
    U_hat, P_hat = UP_hat
    U_hat0, P_hat0 = UP_hat0

    UP = Array(VQ)
    UP0 = Array(VQ)
    U, P = UP
    U0, P0 = UP0

    # RK parameters
    a = (8. / 15., 5. / 12., 3. / 4.)
    b = (0.0, -17. / 60., -5. / 12.)

    # primary variable
    u = UP_hat

    H_hat = Function(VFS)

    dU = Function(VQ)
    hv = np.zeros((2, ) + H_hat.shape, dtype=np.complex)

    Source = Array(
        VFS)  # Note - not using VQ. Only used for constant pressure gradient
    Sk = Function(VFS)

    K2 = K[1] * K[1] + K[2] * K[2]

    for i in range(3):
        K[i] = K[i].astype(float)

    work = work_arrays()
    u_dealias = Array(VFSp)
    curl_hat = Function(VCp)
    curl_dealias = Array(VCp)

    nu, dt, N = params.nu, params.dt, params.N

    up = TrialFunction(VQ)
    vq = TestFunction(VQ)

    ut, pt = up
    vt, qt = vq

    M = []
    for rk in range(3):
        a0 = inner(vt, (2. / nu / dt / (a[rk] + b[rk])) * ut - div(grad(ut)))
        a1 = inner(vt, (2. / nu / (a[rk] + b[rk])) * grad(pt))
        a2 = inner(qt, (2. / nu / (a[rk] + b[rk])) * div(ut))
        M.append(BlockMatrix(a0 + a1 + a2))

    # Collect all matrices
    if ST.family() == 'chebyshev':
        mat = config.AttributeDict(
            dict(AB=[
                HelmholtzCoeff(N[0], 1.,
                               -(K2 - 2. / nu / dt / (a[rk] + b[rk])), 0,
                               ST.quad) for rk in range(3)
            ], ))
    else:
        mat = config.AttributeDict(
            dict(ADD=inner_product((ST, 0), (ST, 2)),
                 BDD=inner_product((ST, 0), (ST, 0))))

    la = None

    hdf5file = CoupledRK3File(config.params.solver,
                              checkpoint={
                                  'space': VQ,
                                  'data': {
                                      '0': {
                                          'UP': [UP_hat]
                                      }
                                  }
                              },
                              results={
                                  'space': VFS,
                                  'data': {
                                      'U': [U]
                                  }
                              })

    del rk
    return config.AttributeDict(locals())
コード例 #2
0
ファイル: KMM.py プロジェクト: minhbau/spectralDNS
def get_context():
    """Set up context for solver"""

    # Get points and weights for Chebyshev weighted integrals
    assert params.Dquad == params.Bquad
    collapse_fourier = False if params.dealias == '3/2-rule' else True
    ST = Basis(params.N[0], 'C', bc=(0, 0), quad=params.Dquad)
    SB = Basis(params.N[0], 'C', bc='Biharmonic', quad=params.Bquad)
    CT = Basis(params.N[0], 'C', quad=params.Dquad)
    ST0 = Basis(params.N[0], 'C', bc=(0, 0), quad=params.Dquad) # For 1D problem
    K0 = Basis(params.N[1], 'F', domain=(0, params.L[1]), dtype='D')
    K1 = Basis(params.N[2], 'F', domain=(0, params.L[2]), dtype='d')

    kw0 = {'threads': params.threads,
           'planner_effort': params.planner_effort["dct"],
           'slab': (params.decomposition == 'slab'),
           'collapse_fourier': collapse_fourier}
    FST = TensorProductSpace(comm, (ST, K0, K1), **kw0)    # Dirichlet
    FSB = TensorProductSpace(comm, (SB, K0, K1), **kw0)    # Biharmonic
    FCT = TensorProductSpace(comm, (CT, K0, K1), **kw0)    # Regular Chebyshev
    VFS = VectorTensorProductSpace([FSB, FST, FST])
    VFST = VectorTensorProductSpace([FST, FST, FST])
    VUG = MixedTensorProductSpace([FSB, FST])
    VCT = VectorTensorProductSpace(FCT)

    mask = FST.get_mask_nyquist() if params.mask_nyquist else None

    # Padded
    kw = {'padding_factor': 1.5 if params.dealias == '3/2-rule' else 1,
          'dealias_direct': params.dealias == '2/3-rule'}
    if params.dealias == '3/2-rule':
        # Requires new bases due to planning and transforms on different size arrays
        STp = Basis(params.N[0], 'C', bc=(0, 0), quad=params.Dquad)
        SBp = Basis(params.N[0], 'C', bc='Biharmonic', quad=params.Bquad)
        CTp = Basis(params.N[0], 'C', quad=params.Dquad)
    else:
        STp, SBp, CTp = ST, SB, CT
    K0p = Basis(params.N[1], 'F', dtype='D', domain=(0, params.L[1]), **kw)
    K1p = Basis(params.N[2], 'F', dtype='d', domain=(0, params.L[2]), **kw)
    FSTp = TensorProductSpace(comm, (STp, K0p, K1p), **kw0)
    FSBp = TensorProductSpace(comm, (SBp, K0p, K1p), **kw0)
    FCTp = TensorProductSpace(comm, (CTp, K0p, K1p), **kw0)
    VFSp = VectorTensorProductSpace([FSBp, FSTp, FSTp])

    float, complex, mpitype = datatypes("double")

    # Mesh variables
    X = FST.local_mesh(True)
    x0, x1, x2 = FST.mesh()
    K = FST.local_wavenumbers(scaled=True)

    # Solution variables
    U = Array(VFS)
    U0 = Array(VFS)
    U_hat = Function(VFS)
    U_hat0 = Function(VFS)
    g = Function(FST)

    # primary variable
    u = (U_hat, g)

    H_hat = Function(VFST)
    H_hat0 = Function(VFST)
    H_hat1 = Function(VFST)

    dU = Function(VFS)
    hv = Function(FSB)
    hg = Function(FST)
    Source = Array(VFS)
    Sk = Function(VFS)

    K2 = K[1]*K[1]+K[2]*K[2]
    K4 = K2**2

    K_over_K2 = np.zeros((2,)+g.shape)
    for i in range(2):
        K_over_K2[i] = K[i+1] / np.where(K2 == 0, 1, K2)

    for i in range(3):
        K[i] = K[i].astype(float)

    work = work_arrays()
    u_dealias = Array(VFSp)
    u0_hat = np.zeros((2, params.N[0]), dtype=complex)
    h0_hat = np.zeros((2, params.N[0]), dtype=complex)
    w = np.zeros((params.N[0], ), dtype=complex)
    w1 = np.zeros((params.N[0], ), dtype=complex)

    nu, dt, N = params.nu, params.dt, params.N

    alfa = K2[0] - 2.0/nu/dt
    # Collect all matrices
    mat = config.AttributeDict(
        dict(CDD=inner_product((ST, 0), (ST, 1)),
             AB=HelmholtzCoeff(N[0], 1., -(K2 - 2.0/nu/dt), 0, ST.quad),
             AC=BiharmonicCoeff(N[0], nu*dt/2., (1. - nu*dt*K2), -(K2 - nu*dt/2.*K4), 0, SB.quad),
             # Matrices for biharmonic equation
             CBD=inner_product((SB, 0), (ST, 1)),
             ABB=inner_product((SB, 0), (SB, 2)),
             BBB=inner_product((SB, 0), (SB, 0)),
             SBB=inner_product((SB, 0), (SB, 4)),
             # Matrices for Helmholtz equation
             ADD=inner_product((ST, 0), (ST, 2)),
             BDD=inner_product((ST, 0), (ST, 0)),
             BBD=inner_product((SB, 0), (ST, 0)),
             CDB=inner_product((ST, 0), (SB, 1)),
             ADD0=inner_product((ST0, 0), (ST0, 2)),
             BDD0=inner_product((ST0, 0), (ST0, 0)),))

    la = config.AttributeDict(
        dict(HelmholtzSolverG=Helmholtz(mat.ADD, mat.BDD, -np.ones((1, 1, 1)),
                                        (K2+2.0/nu/dt)),
             BiharmonicSolverU=Biharmonic(mat.SBB, mat.ABB, mat.BBB, -nu*dt/2.*np.ones((1, 1, 1)),
                                          (1.+nu*dt*K2),
                                          (-(K2 + nu*dt/2.*K4))),
             HelmholtzSolverU0=Helmholtz(mat.ADD0, mat.BDD0, np.array([-1.]), np.array([2./nu/dt])),
             TDMASolverD=TDMA(inner_product((ST, 0), (ST, 0)))))

    hdf5file = KMMFile(config.params.solver,
                       checkpoint={'space': VFS,
                                   'data': {'0': {'U': [U_hat]},
                                            '1': {'U': [U_hat0]}}},
                       results={'space': VFS,
                                'data': {'U': [U]}})

    return config.AttributeDict(locals())
コード例 #3
0
ファイル: MHD.py プロジェクト: ucsky/spectralDNS
def get_context():
    float, complex, mpitype = datatypes(params.precision)
    collapse_fourier = False if params.dealias == '3/2-rule' else True
    dim = len(params.N)
    dtype = lambda d: float if d == dim - 1 else complex
    V = [
        Basis(params.N[i], 'F', domain=(0, params.L[i]), dtype=dtype(i))
        for i in range(dim)
    ]

    kw0 = {
        'threads': params.threads,
        'planner_effort': params.planner_effort['fft']
    }
    T = TensorProductSpace(comm,
                           V,
                           dtype=float,
                           slab=(params.decomposition == 'slab'),
                           collapse_fourier=collapse_fourier,
                           **kw0)
    VT = VectorTensorProductSpace(T)
    VM = MixedTensorProductSpace([T] * 2 * dim)

    mask = T.get_mask_nyquist() if params.mask_nyquist else None

    kw = {
        'padding_factor': 1.5 if params.dealias == '3/2-rule' else 1,
        'dealias_direct': params.dealias == '2/3-rule'
    }

    Vp = [
        Basis(params.N[i], 'F', domain=(0, params.L[i]), dtype=dtype(i), **kw)
        for i in range(dim)
    ]

    Tp = TensorProductSpace(comm,
                            Vp,
                            dtype=float,
                            slab=(params.decomposition == 'slab'),
                            collapse_fourier=collapse_fourier,
                            **kw0)
    VTp = VectorTensorProductSpace(Tp)
    VMp = MixedTensorProductSpace([Tp] * 2 * dim)

    # Mesh variables
    X = T.local_mesh(True)
    K = T.local_wavenumbers(scaled=True)
    for i in range(dim):
        X[i] = X[i].astype(float)
        K[i] = K[i].astype(float)
    K2 = np.zeros(T.shape(True), dtype=float)
    for i in range(dim):
        K2 += K[i] * K[i]

    K_over_K2 = np.zeros(VT.shape(True), dtype=float)
    for i in range(dim):
        K_over_K2[i] = K[i] / np.where(K2 == 0, 1, K2)

    UB = Array(VM)
    P = Array(T)
    curl = Array(VT)
    UB_hat = Function(VM)
    P_hat = Function(T)
    dU = Function(VM)
    Source = Array(VM)
    ub_dealias = Array(VMp)
    ZZ_hat = np.zeros((3, 3) + Tp.shape(True), dtype=complex)  # Work array

    # Create views into large data structures
    U = UB[:3]
    U_hat = UB_hat[:3]
    B = UB[3:]
    B_hat = UB_hat[3:]

    # Primary variable
    u = UB_hat

    hdf5file = MHDFile(config.params.solver,
                       checkpoint={
                           'space': VM,
                           'data': {
                               '0': {
                                   'UB': [UB_hat]
                               }
                           }
                       },
                       results={
                           'space': VM,
                           'data': {
                               'UB': [UB]
                           }
                       })

    return config.AttributeDict(locals())
コード例 #4
0
def get_context():
    """Set up context for solver"""

    # Get points and weights for Chebyshev weighted integrals
    assert params.Dquad == params.Bquad
    collapse_fourier = False if params.dealias == '3/2-rule' else True
    ST = Basis(params.N[0], 'C', bc=(0, 0), quad=params.Dquad)
    CT = Basis(params.N[0], 'C', quad=params.Dquad)
    CP = Basis(params.N[0], 'C', quad=params.Dquad)
    K0 = Basis(params.N[1], 'F', domain=(0, params.L[1]), dtype='D')
    K1 = Basis(params.N[2], 'F', domain=(0, params.L[2]), dtype='d')
    CP.slice = lambda: slice(0, CT.N)

    kw0 = {'threads': params.threads,
           'planner_effort': params.planner_effort["dct"],
           'slab': (params.decomposition == 'slab'),
           'collapse_fourier': collapse_fourier}
    FST = TensorProductSpace(comm, (ST, K0, K1), **kw0)    # Dirichlet
    FCT = TensorProductSpace(comm, (CT, K0, K1), **kw0)    # Regular Chebyshev N
    FCP = TensorProductSpace(comm, (CP, K0, K1), **kw0)    # Regular Chebyshev N-2
    VFS = VectorTensorProductSpace(FST)
    VCT = VectorTensorProductSpace(FCT)
    VQ = MixedTensorProductSpace([VFS, FCP])

    mask = FST.get_mask_nyquist() if params.mask_nyquist else None

    # Padded
    kw = {'padding_factor': 1.5 if params.dealias == '3/2-rule' else 1,
          'dealias_direct': params.dealias == '2/3-rule'}
    if params.dealias == '3/2-rule':
        # Requires new bases due to planning and transforms on different size arrays
        STp = Basis(params.N[0], 'C', bc=(0, 0), quad=params.Dquad)
        CTp = Basis(params.N[0], 'C', quad=params.Dquad)
    else:
        STp, CTp = ST, CT
    K0p = Basis(params.N[1], 'F', dtype='D', domain=(0, params.L[1]), **kw)
    K1p = Basis(params.N[2], 'F', dtype='d', domain=(0, params.L[2]), **kw)
    FSTp = TensorProductSpace(comm, (STp, K0p, K1p), **kw0)
    FCTp = TensorProductSpace(comm, (CTp, K0p, K1p), **kw0)
    VFSp = VectorTensorProductSpace(FSTp)
    VCp = MixedTensorProductSpace([FSTp, FCTp, FCTp])

    float, complex, mpitype = datatypes("double")

    constraints = ((3, 0, 0),
                   (3, params.N[0]-1, 0))

    # Mesh variables
    X = FST.local_mesh(True)
    x0, x1, x2 = FST.mesh()
    K = FST.local_wavenumbers(scaled=True)

    # Solution variables
    UP_hat = Function(VQ)
    UP_hat0 = Function(VQ)
    U_hat, P_hat = UP_hat
    U_hat0, P_hat0 = UP_hat0

    UP = Array(VQ)
    UP0 = Array(VQ)
    U, P = UP
    U0, P0 = UP0

    # primary variable
    u = UP_hat

    H_hat = Function(VFS)
    H_hat0 = Function(VFS)
    H_hat1 = Function(VFS)

    dU = Function(VQ)
    Source = Array(VFS) # Note - not using VQ. Only used for constant pressure gradient
    Sk = Function(VFS)

    K2 = K[1]*K[1]+K[2]*K[2]

    for i in range(3):
        K[i] = K[i].astype(float)

    work = work_arrays()
    u_dealias = Array(VFSp)
    curl_hat = Function(VCp)
    curl_dealias = Array(VCp)

    nu, dt, N = params.nu, params.dt, params.N

    up = TrialFunction(VQ)
    vq = TestFunction(VQ)

    ut, pt = up
    vt, qt = vq

    alfa = 2./nu/dt
    a0 = inner(vt, (2./nu/dt)*ut-div(grad(ut)))
    a1 = inner(vt, (2./nu)*grad(pt))
    a2 = inner(qt, (2./nu)*div(ut))

    M = BlockMatrix(a0+a1+a2)

    # Collect all matrices
    mat = config.AttributeDict(
        dict(CDD=inner_product((ST, 0), (ST, 1)),
             AB=HelmholtzCoeff(N[0], 1., alfa-K2, 0, ST.quad),))

    la = None

    hdf5file = CoupledFile(config.params.solver,
                        checkpoint={'space': VQ,
                                    'data': {'0': {'UP': [UP_hat]},
                                             '1': {'UP': [UP_hat0]}}},
                        results={'space': VFS,
                                 'data': {'U': [U]}})

    return config.AttributeDict(locals())
コード例 #5
0
def get_context():
    """Set up context for classical (NS) solver"""
    float, complex, mpitype = datatypes(params.precision)
    collapse_fourier = False if params.dealias == '3/2-rule' else True
    dim = len(params.N)
    dtype = lambda d: float if d == dim - 1 else complex
    V = [
        FunctionSpace(params.N[i],
                      'F',
                      domain=(0, params.L[i]),
                      dtype=dtype(i)) for i in range(dim)
    ]

    kw0 = {
        'threads': params.threads,
        'planner_effort': params.planner_effort['fft']
    }
    T = TensorProductSpace(comm,
                           V,
                           dtype=float,
                           slab=(params.decomposition == 'slab'),
                           collapse_fourier=collapse_fourier,
                           **kw0)
    VT = VectorSpace(T)

    # Different bases for nonlinear term, either 2/3-rule or 3/2-rule
    kw = {
        'padding_factor': 1.5 if params.dealias == '3/2-rule' else 1,
        'dealias_direct': params.dealias == '2/3-rule'
    }

    Vp = [
        FunctionSpace(params.N[i],
                      'F',
                      domain=(0, params.L[i]),
                      dtype=dtype(i),
                      **kw) for i in range(dim)
    ]

    Tp = TensorProductSpace(comm,
                            Vp,
                            dtype=float,
                            slab=(params.decomposition == 'slab'),
                            collapse_fourier=collapse_fourier,
                            **kw0)
    VTp = VectorSpace(Tp)

    mask = T.get_mask_nyquist() if params.mask_nyquist else None

    # Mesh variables
    X = T.local_mesh(True)
    K = T.local_wavenumbers(scaled=True)
    for i in range(dim):
        X[i] = X[i].astype(float)
        K[i] = K[i].astype(float)
    K2 = np.zeros(T.shape(True), dtype=float)
    for i in range(dim):
        K2 += K[i] * K[i]

    K_over_K2 = np.zeros(VT.shape(True), dtype=float)
    for i in range(dim):
        K_over_K2[i] = K[i] / np.where(K2 == 0, 1, K2)

    # Velocity and pressure. Use ndarray view for efficiency
    U = Array(VT)
    U_hat = Function(VT)
    P = Array(T)
    P_hat = Function(T)
    u_dealias = Array(VTp)

    # Primary variable
    u = U_hat

    # RHS array
    dU = Function(VT)
    curl = Array(VT)
    Source = Function(VT)  # Possible source term initialized to zero
    work = work_arrays()

    hdf5file = NSFile(config.params.solver,
                      checkpoint={
                          'space': VT,
                          'data': {
                              '0': {
                                  'U': [U_hat]
                              }
                          }
                      },
                      results={
                          'space': VT,
                          'data': {
                              'U': [U],
                              'P': [P]
                          }
                      })

    return config.AttributeDict(locals())