To perform a 3D CFD simulation in Python, we can use PyTorch, which is a popular deep learning framework capable of running computations on GPUs. Following are the general steps to perform a CFD simulation in 3D -
- Define the geometry and physical parameters of the problem in 3D using a mesh. There are several meshing libraries available in Python like NumPy, SciPy, and PyMesh.
- Define the initial and boundary conditions based on the problem at hand.
- Implement the numerical schemes to solve the Navier-Stokes equations using finite volume or finite difference methods. For instance, we can solve the equations using the Chorin's projection method.
def solve_Navier_Stokes_projection(u_x, u_y, u_z, rho, mu, dt, dx, dy, dz):
# Solve for velocity(vector)
u = np.vstack((u_x.flatten(), u_y.flatten(), u_z.flatten())).T
# Solve for pressure(scalar)
p = np.zeros((u.shape[0], 1))
# Define Divergence operator
D = scipy.sparse.csr_matrix(3*[scipy.sparse.diags([-1, 1], [0, 1], shape=(Nx, Ny*Nz))])
# Velocity Gradient Matrix
grad = np.vstack((np.kron(np.ones((1, Nx)), np.kron(np.eye(Ny), np.ones((1, Nz))) / dy),
np.kron(np.ones((1, Nx)), np.kron(np.ones((1, Ny)), np.eye(Nz)) / dz)))
grad = scipy.sparse.csr_matrix(grad)
# Define Laplacian Operator
lapl = scipy.sparse.diags([1, 1, 1, -6, 1, 1, 1], [-Nx*Ny, -Nx, -1, 0, 1, Nx, Nx*Ny],
shape=(Nx*Ny*Nz, Nx*Ny*Nz)) * mu / dx**2
# Calculate modified velocity
rhs = u / dt - grad.dot(p) + ( D.dot(u.flatten())) * mu / rho
u_star = lgmres(lapl, rhs)[0].reshape((Nx,Ny,Nz,3)).T
# Pressure Correction (Poisson Equation)
div = np.vstack((np.kron(np.ones((1, Nx)), np.kron(np.eye(Ny), np.ones((1, Nz))) * dy),
np.kron(np.ones((1, Nx)), np.kron(np.ones((1, Ny)), np.eye(Nz))) * dz ))
div = scipy.sparse.csr_matrix(div)
A = div.dot(scipy.sparse.diags([-1, -1, -1], [0, Nx*Ny, Nx*Ny*Nz],
shape=(Nx*Ny*Nz, Nx*Ny*Nz)).toarray())
b = -div.dot(np.vstack((u_star[0,:,:,:]/dx[0],
u_star[1,:,:,:]/dx[1],
u_star[2,:,:,:]/dx[2]))).flatten(order='F') / dt
# Pressure Correction
p_prime = lgmres(A, b)[0].reshape((Nx,Ny,Nz)).T
# Correct Velocity Field
u_x[:, :, :] = u_star[0,:,:,:] - dt / dx[0] * (p_prime[1:, :, :] - p_prime[:-1, :, :])
u_y[:, :, :] = u_star[1,:,:,:] - dt / dy * (p_prime[:, 1:, :] - p_prime[:, :-1, :])
u_z[:, :, :] = u_star[2,:,:,:] - dt / dz * (p_prime[:, :, 1:] - p_prime[:, :, :-1])
return u_x, u_y, u_z
- Iterate over time steps to calculate the final solution.
- Visualize the results using various visualization libraries like Matplotlib, Mayavi, and PyVista.
import pyvista as pv
def visualize_flow(u_x, u_y, u_z, fig_width=10, fig_height=7, axs=None):
# Create a new plot
if axs is None:
axs = pv.Plotter(window_size=[int(fig_width*80), int(fig_height*80)])
# Create a vector field data
vectors = np.stack((u_x, u_y, u_z), axis=-1)
# create grid mesh from data
mesh = pv.StructuredGrid(X, Y, Z)
mesh.point_arrays['vector'] = vectors.reshape((-1, 3), order='F')
# add vector field actor
actor = axs.add_mesh(mesh, scalars='vector',
vector_scalars='Magnitude',
n_colors=256,
cmap='viridis',
lighting=True,
scalar_bar_args={'title': 'Velocity Magnitude\n[m/s]',
'n_labels': 5,
'height': 0.50,
'position_x': 0.95,
'position_y': 0.45},
scalar_bar_height_ratio=0.75,
name='VectorField'
)
# add streamlines actor
stream_actor = actor.streamlines(color='white',
integration_direction='backwards',
source_radius=0.02,
tube_radius=0.005,
max_time=2.0,
initial_step_length=0.1,
start_position=(-0.5, 0.0, 0.0),
name="Streamlines")
# set camera position
axs.camera_position = [(45, 45, 57), (-0.5, 0.0, 0.0), (0.0, 0.0, 1.0)]
# Render the image
axs.show(True)
return axs
The above code is a general template that can be used to perform 3D CFD simulations. This can be further modified or optimized based on specific problem requirements.