API Reference

Contents

API Reference#

Pre-processing scripts#

vasp.automatedPreprocessing.automated_preprocessing.main_meshing()[source]#
vasp.automatedPreprocessing.automated_preprocessing.read_command_line(input_path=None)[source]#

Read arguments from commandline and return all values in a dictionary. If input_path is not None, then do not parse command line, but only return default values.

Args:

input_path (str): Input file path, positional argument with default None.

vasp.automatedPreprocessing.automated_preprocessing.run_pre_processing(input_model, verbose_print, smoothing_method, smoothing_factor, smoothing_iterations, meshing_method, refine_region, has_multiple_inlets, add_flow_extensions, visualize, config_path, coarsening_factor, inlet_flow_extension_length, outlet_flow_extension_length, number_of_sublayers_fluid, number_of_sublayers_solid, edge_length, region_points, compress_mesh, scale_factor, scale_factor_h5, resampling_step, meshing_parameters, remove_all, solid_thickness, solid_thickness_parameters, mesh_format, flow_rate_factor, solid_side_wall_id, interface_fsi_id, solid_outer_wall_id, fluid_volume_id, solid_volume_id, mesh_generation_retries, no_solid, extract_branch, branch_group_ids, branch_ids_offset, distance_method)[source]#

Automatically generate mesh of surface model in .vtu and .xml format, including prescribed flow rates at inlet and outlet based on flow network model.

Runs simulation of meshed case on a remote ssh server if server configuration is provided.

Parameters:
  • input_model (str) – Name of case

  • verbose_print (bool) – Toggles verbose mode

  • smoothing_method (str) – Method for surface smoothing

  • smoothing_factor (float) – Smoothing factor of Voronoi smoothing

  • smoothing_iterations (int) – Number of smoothing iterations for Taubin and Laplace smoothing

  • meshing_method (str) – Determines what the density of the volumetric mesh depends upon

  • refine_region (bool) – Refines selected region of input if True

  • has_multiple_inlets (bool) – Specifies whether the input model has multiple inlets

  • add_flow_extensions (bool) – Adds flow extensions to mesh if True

  • visualize (bool) – Visualize resulting surface model with flow rates

  • config_path (str) – Path to configuration file for remote simulation

  • coarsening_factor (float) – Refine or coarsen the standard mesh size with given factor

  • inlet_flow_extension_length (float) – Factor defining length of flow extensions at the inlet(s)

  • outlet_flow_extension_length (float) – Factor defining length of flow extensions at the outlet(s)

  • number_of_sublayers_fluid (int) – Number of sublayers for fluid

  • number_of_sublayers_solid (int) – Number of sublayers for solid

  • edge_length (float) – Edge length used for meshing with constant element size

  • region_points (list) – User defined points to define which region to refine

  • compress_mesh (bool) – Compresses finalized mesh if True

  • scale_factor (float) – Scale input model by this factor

  • resampling_step (float) – Float value determining the resampling step for centerline computations, in [m]

  • meshing_parameters (list) – Parameters for meshing method ‘distancetospheres’

  • remove_all (bool) – Remove mesh and all pre-processing files

  • solid_thickness (str) – Constant or variable mesh thickness

  • solid_thickness_parameters (list) – Specify parameters for solid thickness

  • mesh_format (str) – Specify the format for the generated mesh

  • flow_rate_factor (float) – Flow rate factor

  • solid_side_wall_id (int) – ID for solid side wall

  • interface_fsi_id (int) – ID for the FSI interface

  • solid_outer_wall_id (int) – ID for the solid outer wall

  • fluid_volume_id (int) – ID for the fluid volume

  • solid_volume_id (int) – ID for the solid volume

  • mesh_generation_retries (int) – Number of mesh generation retries before trying alternative method

  • no_solid (bool) – Generate mesh without solid

  • extract_branch (bool) – Enable extraction of a specific branch, marking solid mesh IDs with an offset.

  • branch_group_ids (list) – Specify group IDs to extract for the branch.

  • branch_ids_offset (int) – Set offset for marking solid mesh IDs when extracting a branch.

  • distance_method (str) – Change between ‘euclidean’ and ‘geodesic’ distance measure

vasp.automatedPreprocessing.preprocessing_common.convert_vtu_mesh_to_xdmf(file_name_vtu_mesh: str | Path, file_name_xdmf_mesh: str | Path) None[source]#

Convert a VTU mesh to XDMF format using meshio. This function is intended to run in serial.

Parameters:
  • file_name_vtu_mesh (Union[str, Path]) – Path to the input VTU mesh file.

  • file_name_xdmf_mesh (Union[str, Path]) – Path to the output XDMF file.

vasp.automatedPreprocessing.preprocessing_common.convert_xml_mesh_to_hdf5(file_name_xml_mesh: str | Path, scaling_factor: float = 1) None[source]#

Converts an XML mesh to an HDF5 mesh.

Parameters:
  • file_name_xml_mesh (Union[str, Path]) – The name of the XML mesh file.

  • scaling_factor (float, optional) – A scaling factor to apply to the mesh coordinates. The default value is 1 (no scaling). Note that probes and parameters inside _info.json file will not be scaled if you only scale HDF5 file.

Returns:

None

Raises:

FileNotFoundError – If the XML mesh file does not exist.

vasp.automatedPreprocessing.preprocessing_common.dist_sphere_spheres(surface: vtkPolyData, save_path: str | Path, distance_offset: float, distance_scale: float, min_distance: float, max_distance: float, distance_method: str = 'geodesic') vtkPolyData[source]#

Determines the target edge length for each cell on the surface, including potential refinement or coarsening of certain user specified areas. Level of refinement/coarseness is determined based on the distance to the spheres. The distance computation can be either ‘euclidean’ or ‘geodesic’ (default).

Parameters:
  • surface (vtkPolyData) – Input surface model

  • save_path (Union[str, Path]) – Location to store processed surface

  • distance_offset (float) – Offset added to the distances

  • distance_scale (float) – Scale applied to the distances

  • min_distance (float) – Minimum value for the distances

  • max_distance (float) – Maximum value for the distances

  • distance_method (str) – Method to compute distances (‘euclidean’ or ‘geodesic’)

Returns:

Processed surface model with info on cell specific target edge length

Return type:

surface (vtkPolyData)

vasp.automatedPreprocessing.preprocessing_common.distance_to_spheres_solid_thickness(surface: vtkPolyData, save_path: str | Path, distance_offset: float = 0, distance_scale: float = 0.1, min_distance: float = 0.25, max_distance: float = 0.3) vtkPolyData[source]#

Determines the solid thickness using vmtkdistancetospheres.

Parameters:
  • surface (vtkPolyData) – Input surface model

  • save_path (Union[str, Path]) – Location to store processed surface

  • distance_offset (float) – Offset added to the distances

  • distance_scale (float) – Scale applied to the distances

  • min_distance (float) – Minimum value for the distances

  • max_distance (float) – Maximum value for the distances

Returns:

Processed surface model with info on solid thickness

Return type:

surface (vtkPolyData)

vasp.automatedPreprocessing.preprocessing_common.edge_length_evaluator(file_name_mesh: str | Path, file_name_edge_length_xdmf: str | Path) None[source]#

Evaluates the edge length of a mesh.

Parameters:
  • file_name_mesh (Union[str, Path]) – Path to the XML mesh file.

  • file_name_edge_length_xdmf (Union[str, Path]) – Path to the output XDMF file.

vasp.automatedPreprocessing.preprocessing_common.generate_mesh(surface: vtkPolyData, number_of_sublayers_fluid: int, number_of_sublayers_solid: int, solid_thickness: str, solid_thickness_parameters: list, centerlines: vtkPolyData, solid_side_wall_id: int = 11, interface_fsi_id: int = 22, solid_outer_wall_id: int = 33, fluid_volume_id: int = 0, solid_volume_id: int = 1, no_solid: bool = False, extract_branch: bool = False, branch_group_ids: list = [], branch_ids_offset: int = 1000) tuple[source]#

Generates a mesh suitable for FSI from an input surface model.

Parameters:
  • surface (vtkPolyData) – Surface model to be meshed.

  • number_of_sublayers_fluid (int) – Number of sublayers for fluid.

  • number_of_sublayers_solid (int) – Number of sublayers for solid.

  • solid_thickness (str) – Type of solid thickness (‘variable’ or ‘constant’).

  • solid_thickness_parameters (list) – List of parameters for solid thickness.

  • centerlines (vtkPolyData) – Centerlines of input model.

  • solid_side_wall_id (int, optional) – ID for solid side wall. Default is 11.

  • interface_fsi_id (int, optional) – ID for the FSI interface. Default is 22.

  • solid_outer_wall_id (int, optional) – ID for solid outer wall. Default is 33.

  • fluid_volume_id (int, optional) – ID for the fluid volume. Default is 0.

  • solid_volume_id (int, optional) – ID for the solid volume. Default is 1.

  • no_solid (bool, optional) – Generate mesh without solid.

  • extract_branch (bool, optional) – Enable extraction of a specific branch, marking solid mesh IDs with an offset.

  • branch_group_ids (list, optional) – Specify group IDs to extract for the branch.

  • branch_ids_offset (int) – Set offset for marking solid mesh IDs when extracting a branch.

Returns:

A tuple containing the generated mesh (vtkUnstructuredGrid) and the remeshed surface (vtkPolyData).

Return type:

tuple

class vasp.automatedPreprocessing.vmtkmeshgeneratorfsi.vmtkMeshGeneratorFsi[source]#

Bases: pypeScript

Execute()[source]#

Post-processing scripts#

This script is a versatile Python script for parsing and visualizing simulation log files. It extracts data from log files, offers flexible plotting options, and helps users gain insights from simulation results.

Example:

vasp-log-plotter simulation.log –plot-all –save –output-directory Results –figure-size 12,8

vasp.automatedPostprocessing.log_plotter.compute_average_over_cycles(data: ndarray, time_steps_per_cycle: int) ndarray[source]#

Compute the average over cycles in a numpy array.

Parameters:
  • data (np.ndarray) – The input data array.

  • time_steps_per_cycle (int) – The number of time steps in each cycle.

Returns:

A numpy array containing the average data over cycles.

Return type:

np.ndarray

vasp.automatedPostprocessing.log_plotter.compute_tke(probe_points: Dict[int, Dict[str, Any]], time_steps_per_cycle: int, start_cycle: int | None = None, end_cycle: int | None = None) Dict[int, Tuple[ndarray, ndarray, ndarray]][source]#

Compute the mean velocity, fluctuating velocity, and turbulent kinetic energy for each point within the specified cycle range in the probe points data using phase-averaging.

Parameters:
  • probe_points (dict) – Probe points data as returned by parse_log_file.

  • time_steps_per_cycle (int) – Number of time steps per cycle.

  • start_cycle (int, optional) – The cycle to start computing from (inclusive). Default is the first cycle.

  • end_cycle (int, optional) – The cycle to end computing at (inclusive). Default is the last cycle.

Returns:

A dictionary containing the mean velocity, fluctuating velocity, and TKE for each point within the

specified cycle range. Each entry is a tuple of (mean_velocity, fluctuating_velocity, tke_array).

Return type:

dict

vasp.automatedPostprocessing.log_plotter.main() None[source]#
vasp.automatedPostprocessing.log_plotter.parse_command_line_args() Namespace[source]#

Parse command-line arguments.

Returns:

Parsed command-line arguments.

Return type:

argparse.Namespace

vasp.automatedPostprocessing.log_plotter.parse_dictionary_from_log(log_file: str) dict[source]#

Parse a dictionary-like content from a log file and return it as a dictionary.

Parameters:

log_file (str) – Path to the log file.

Returns:

Parsed dictionary.

Return type:

dict

vasp.automatedPostprocessing.log_plotter.parse_log_file(log_file: str) Dict[str, Any][source]#

Parse a log file and store data in a structured dictionary with numpy arrays.

Parameters:

log_file (str) – Path to the log file.

Returns:

A dictionary containing the parsed data.

Return type:

dict

vasp.automatedPostprocessing.log_plotter.plot_multiple_variables_comparison(variable_mean: ndarray, variable_min: ndarray, variable_max: ndarray, variable_name: str, time_steps_per_cycle: int, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (10, 6), start_cycle: int | None = 1, end_cycle: int | None = None) None[source]#

Plot mean, min, and max variables against time on the same figure.

Parameters:
  • variable_mean (numpy.ndarray) – Array containing the mean variable values.

  • variable_min (numpy.ndarray) – Array containing the min variable values.

  • variable_max (numpy.ndarray) – Array containing the max variable values.

  • variable_name (str) – Names of the variables for labeling the plot (mean, min, max).

  • time_steps_per_cycle (int) – The number of time steps in each cycle.

  • save_to_file (bool, optional) – Whether to save the figure to a file (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (10, 6).

  • start_cycle (int, optional) – The cycle to start comparing from. Default is 1 (start from first cycle).

  • end_cycle (int, optional) – The cycle to end comparing at. Default is None (end at last cycle).

vasp.automatedPostprocessing.log_plotter.plot_multiple_variables_vs_time(time: ndarray, variable_mean: ndarray, variable_min: ndarray, variable_max: ndarray, variable_name: str, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (10, 6), start: int | None = None, end: int | None = None) None[source]#

Plot mean, min, and max variables against time on the same figure.

Parameters:
  • time (numpy.ndarray) – Array containing time values.

  • variable_mean (numpy.ndarray) – Array containing the mean variable values.

  • variable_min (numpy.ndarray) – Array containing the min variable values.

  • variable_max (numpy.ndarray) – Array containing the max variable values.

  • variable_name (str) – Names of the variables for labeling the plot (mean, min, max).

  • save_to_file (bool, optional) – Whether to save the figure to a file (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (10, 6).

  • start (int, optional) – Index to start plotting data from. Default is None (start from the beginning).

  • end (int, optional) – Index to end plotting data at. Default is None (end at the last data point).

vasp.automatedPostprocessing.log_plotter.plot_newton_iteration(variable: ndarray, variable_name: str, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (10, 6)) None[source]#

Plot Newton iteration (atol or rtol).

Parameters:
  • variable (numpy.ndarray) – Array containing the variable values.

  • variable_name (str) – Name of the variable for labeling the plot.

  • save_to_file (bool, optional) – Whether to save the figure to a file (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (10, 6).

vasp.automatedPostprocessing.log_plotter.plot_probe_points(time: ndarray, probe_points: Dict[int, Dict[str, ndarray]], selected_probe_points: List[int] | None = None, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (12, 6), start: int | None = None, end: int | None = None) None[source]#

Plot velocity magnitude and pressure for probe points against time.

Parameters:
  • time (numpy.ndarray) – Time array.

  • probe_points (dict) – Probe point data containing velocity magnitude and pressure arrays.

  • selected_probe_points (list, optional) – List of probe points to plot. Plot all probe points if not provided.

  • save_to_file (bool, optional) – Whether to save the figures to files (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (12, 8).

  • start (int, optional) – Index to start plotting data from. Default is None (start from the beginning).

  • end (int, optional) – Index to end plotting data at. Default is None (end at the last data point).

vasp.automatedPostprocessing.log_plotter.plot_probe_points_comparison(probe_points: Dict[int, Dict[str, ndarray]], time_steps_per_cycle: int, selected_probe_points: List[int] | None = None, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (12, 6), start_cycle: int | None = 0, end_cycle: int | None = None) None[source]#

Plot comparison of velocity magnitude and pressure for probe points across multiple cycles.

Parameters:
  • probe_points (dict) – Probe point data containing velocity magnitude and pressure arrays.

  • selected_probe_points (list, optional) – List of probe points to plot. Plot all probe points if not provided.

  • time_steps_per_cycle (int) – The number of time steps in each cycle.

  • save_to_file (bool, optional) – Whether to save the figures to files (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (12, 8).

  • start_cycle (int, optional) – The cycle to start comparing from. Default is 1 (start from first cycle).

  • end_cycle (int, optional) – The cycle to end comparing at. Default is None (end at last cycle).

vasp.automatedPostprocessing.log_plotter.plot_probe_points_displacement(time: ndarray, probe_points: Dict[int, Dict[str, ndarray]], selected_probe_points: List[int] | None = None, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (12, 6), start: int | None = None, end: int | None = None) None[source]#

Plot displacement magnitude for probe points against time.

Parameters:
  • time (numpy.ndarray) – Time array.

  • probe_points (dict) – Probe point data containing displacement magnitude arrays.

  • selected_probe_points (list, optional) – List of probe points to plot. Plot all probe points if not provided.

  • save_to_file (bool, optional) – Whether to save the figures to files (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (12, 8).

  • start (int, optional) – Index to start plotting data from. Default is None (start from the beginning).

  • end (int, optional) – Index to end plotting data at. Default is None (end at the last data point).

vasp.automatedPostprocessing.log_plotter.plot_probe_points_displacement_comparison(probe_points: Dict[int, Dict[str, ndarray]], time_steps_per_cycle: int, selected_probe_points: List[int] | None = None, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (12, 6), start_cycle: int | None = 0, end_cycle: int | None = None) None[source]#

Plot comparison of displacement magnitude for probe points across multiple cycles.

Parameters:
  • probe_points (dict) – Probe point data containing displacement magnitude arrays.

  • selected_probe_points (list, optional) – List of probe points to plot. Plot all probe points if not provided.

  • time_steps_per_cycle (int) – The number of time steps in each cycle.

  • save_to_file (bool, optional) – Whether to save the figures to files (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (12, 8).

  • start_cycle (int, optional) – The cycle to start comparing from. Default is 1 (start from first cycle).

  • end_cycle (int, optional) – The cycle to end comparing at. Default is None (end at last cycle).

vasp.automatedPostprocessing.log_plotter.plot_probe_points_tke(tke_data: Dict[int, Tuple[ndarray, ndarray, ndarray]], selected_probe_points: List[int] | None = None, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (12, 6), start: int | None = None, end: int | None = None)[source]#

Plot the turbulent kinetic energy (TKE) for each probe point in separate subplots.

Parameters:
  • tke_data (dict) – A dictionary containing TKE data for each probe point. This should be in the format returned by compute_mean_fluctuating_and_tke_velocity.

  • save_to_file (bool, optional) – Whether to save the figures to files (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (12, 8).

  • start (int, optional) – Index to start plotting data from. Default is None (start from the beginning).

  • end (int, optional) – Index to end plotting data at. Default is None (end at the last data point).

vasp.automatedPostprocessing.log_plotter.plot_probe_points_tke_comparison(tke_data: Dict[int, Tuple[ndarray, ndarray, ndarray]], time_steps_per_cycle: int, selected_probe_points: List[int] | None = None, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (12, 6))[source]#

Plot the turbulent kinetic energy (TKE) per cycle for selected probe points in separate figures.

Parameters:
  • tke_data (dict) – A dictionary containing TKE data for each probe point. This should be in the format returned by compute_tke.

  • time_steps_per_cycle (int) – Number of time steps per cycle.

  • selected_probe_points (list, optional) – List of probe points to plot. If not provided, all probe points will be plotted.

  • save_to_file (bool, optional) – Whether to save the figures to files (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (12, 8).

vasp.automatedPostprocessing.log_plotter.plot_variable_comparison(variable: ndarray, variable_name: str, time_steps_per_cycle: int, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (10, 6), start_cycle: int | None = 1, end_cycle: int | None = None) None[source]#

Plot comparison of a variable across multiple cycles.

Parameters:
  • variable (numpy.ndarray) – Array containing the variable values.

  • variable_name (str) – Name of the variable for labeling the plot.

  • time_steps_per_cycle (int) – The number of time steps in each cycle.

  • save_to_file (bool, optional) – Whether to save the figure to a file (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (10, 6).

  • start_cycle (int, optional) – The cycle to start comparing from. Default is 1 (start at first cycle).

  • end_cycle (int, optional) – The cycle to end comparing at. Default is None (end at last cycle).

vasp.automatedPostprocessing.log_plotter.plot_variable_vs_time(time: ndarray, variable: ndarray, variable_name: str, save_to_file: bool = False, output_directory: str | None = None, figure_size: Tuple[int, int] = (10, 6), start: int | None = None, end: int | None = None) None[source]#

Plot a variable against time.

Parameters:
  • time (numpy.ndarray) – Array containing time values.

  • variable (numpy.ndarray) – Array containing the variable values.

  • variable_name (str) – Name of the variable for labeling the plot.

  • save_to_file (bool, optional) – Whether to save the figure to a file (default is False).

  • output_directory (str, optional) – The directory where the figure will be saved when save_to_file is True.

  • figure_size (tuple, optional) – Figure size in inches (width, height). Default is (10, 6).

  • start (int, optional) – Index to start plotting data from. Default is None (start from the beginning).

  • end (int, optional) – Index to end plotting data at. Default is None (end at the last data point).

vasp.automatedPostprocessing.log_plotter.save_plot_to_file(variable_name: str, output_directory: str | None) None[source]#

Save a plot to a file.

Parameters:
  • variable_name (str) – Name of the variable for generating the filename.

  • output_directory (str, optional) – The directory where the figure will be saved.

vasp.automatedPostprocessing.log_plotter.save_probe_points_data_to_file(probe_points: Dict[int, Dict[str, ndarray]], output_directory: str | None, time: ndarray, start: int | None = None, end: int | None = None) None[source]#

Save probe points data to files.

Parameters:
  • probe_points (dict) – Probe point data containing velocity magnitude and pressure arrays.

  • output_directory (str, optional) – The directory where the files will be saved when save_to_file is True.

  • time (numpy.ndarray) – Time array.

  • start (int, optional) – Index to start saving data from. Default is None (start from the beginning).

  • end (int, optional) – Index to end saving data at. Default is None (end at the last data point).

vasp.automatedPostprocessing.log_plotter.save_probe_points_displacement_data_to_file(probe_points: Dict[int, Dict[str, ndarray]], output_directory: str | None, time: ndarray, start: int | None = None, end: int | None = None) None[source]#

Save probe points displacement data to files.

Parameters:
  • probe_points (dict) – Probe point data containing displacement magnitude arrays.

  • output_directory (str, optional) – The directory where the files will be saved when save_to_file is True.

  • time (numpy.ndarray) – Time array.

  • start (int, optional) – Index to start saving data from. Default is None (start from the beginning).

  • end (int, optional) – Index to end saving data at. Default is None (end at the last data point).

This script is used to predeform the mesh for an FSI simulation. It assumes that the simulation has already been executed, and the displacement information is available in the ‘displacement.h5’ file. By applying the reverse of the displacement to the original mesh, this script generates a predeformed mesh for subsequent simulation steps.

vasp.automatedPostprocessing.predeform_mesh.main() None[source]#

Main function for parsing arguments and predeforming the mesh.

Returns:

None

vasp.automatedPostprocessing.predeform_mesh.parse_arguments() Namespace[source]#

Parse command line arguments.

Returns:

Parsed command-line arguments.

Return type:

argparse.Namespace

vasp.automatedPostprocessing.predeform_mesh.predeform_mesh(folder_path: Path, mesh_path: Path, scale_factor: float) None[source]#

Predeform the mesh for FSI simulation.

Parameters:
  • folder_path (Path) – Path to the simulation results folder.

  • mesh_path (Path) – Path to the mesh file.

  • scale_factor (float) – Scale factor for mesh deformation.

Returns:

None

vasp.automatedPostprocessing.postprocessing_common.get_domain_ids(mesh_path, fluid_domain_id, solid_domain_id)[source]#

Given a mesh file, this function returns the IDs of the fluid and solid domains

Parameters:
  • mesh_path (Path) – Path to the mesh file that contains the fluid and solid domains

  • fluid_domain_id (int) – ID of the fluid domain

  • solid_domain_id (int) – ID of the solid domain

Returns:

List of IDs of the fluid domain solid_ids (list): List of IDs of the solid domain all_ids (list): List of IDs of the whole mesh

Return type:

fluid_ids (list)

vasp.automatedPostprocessing.postprocessing_common.output_file_lists(xdmf_file: Path) Tuple[List[str], List[float], List[int]][source]#

If the simulation has been restarted, the output is stored in multiple files and may not have even temporal spacing This loop determines the file names from the xdmf output file

Parameters:

xdmf_file (Path) – Path to xdmf file

Returns:

A tuple containing:
  • List of names of h5 files associated with each timestep

  • List of time values in xdmf file

  • List of indices of each timestep in the corresponding h5 file

Return type:

Tuple[List[str], List[float], List[int]]

vasp.automatedPostprocessing.postprocessing_common.read_parameters_from_file(folder: str | Path) Dict | None[source]#

Reads parameters from a JSON file located in the specified folder.

Parameters:

folder (str) – The folder containing simulation results

Returns:

The loaded parameters as a Python dictionary, or None if an error occurs.

Return type:

dict or None

This script reads the displacement and velocity data from turtleFSI output and reformats the data so that it can be read in fenics. The output files are saved in the Visualization_separate_domain folder.

vasp.automatedPostprocessing.postprocessing_fenics.create_hdf5.create_hdf5(visualization_path, mesh_path, save_time_step, stride, start_time, end_time, extract_solid_only, fluid_domain_id, solid_domain_id)[source]#

Loads displacement/velocity data from turtleFSI output and reformats the data so that it can be read in fenics.

Parameters:
  • visualization_path (Path) – Path to the folder containing the visualization files (displacement/velocity.h5)

  • mesh_path (Path) – Path to the mesh file (mesh.h5 or mesh_refined.h5 depending on save_deg)

  • stride – stride of the time steps to be saved

  • start_t (float) – desired start time for the output file

  • end_t (float) – desired end time for the output file

  • extract_solid_only (bool) – If True, only the solid domain is extracted for displacement. If False, both the fluid and solid domains are extracted.

  • fluid_domain_id (int or list) – ID of the fluid domain

  • solid_domain_id (int or list) – ID of the solid domain

vasp.automatedPostprocessing.postprocessing_fenics.create_hdf5.main() None[source]#
vasp.automatedPostprocessing.postprocessing_fenics.create_hdf5.parse_arguments() Namespace[source]#

Parse command line arguments.

Returns:

Parsed command-line arguments.

Return type:

argparse.Namespace

This script loads displacement and velocity from .h5 file given by create_hdf5.py, converts and saves to .xdmf format for visualization (in e.g. ParaView).

vasp.automatedPostprocessing.postprocessing_fenics.create_separate_domain_visualization.create_separate_domain_visualization(visualization_separate_domain_folder, mesh_path, stride=1)[source]#

Loads displacement and velocity from .h5 file given by create_hdf5.py, converts and saves to .xdmf format for visualization (in e.g. ParaView). This function works with MPI. If the displacement was saved for the entire domain, no additional xdmf file will be created for the displacement. :param visualization_separate_domain_folder: Path to the folder containing the .h5 files :type visualization_separate_domain_folder: Path :param mesh_path: Path to the mesh that contains both fluid and solid domain :type mesh_path: Path :param stride: Save frequency of visualization output (default: 1) :type stride: int

vasp.automatedPostprocessing.postprocessing_fenics.create_separate_domain_visualization.main() None[source]#
vasp.automatedPostprocessing.postprocessing_fenics.create_separate_domain_visualization.parse_arguments() Namespace[source]#

Parse command line arguments.

Returns:

Parsed command-line arguments.

Return type:

argparse.Namespace

common functions for postprocessing-fenics scripts

vasp.automatedPostprocessing.postprocessing_fenics.postprocessing_fenics_common.parse_arguments() Namespace[source]#

Parse command line arguments.

Returns:

Parsed command-line arguments.

Return type:

argparse.Namespace

vasp.automatedPostprocessing.postprocessing_fenics.postprocessing_fenics_common.project_dg(f: Function, V: FunctionSpace) Function[source]#

Project a function v into a DG space V. It perfomrs the same operation as dolfin.project, but it is more efficient since we use local_solver which is possible since we use DG spaces.

Parameters:
  • v (Function) – Function to be projected

  • V (FunctionSpace) – DG space

Returns:

Projected function

Return type:

Function

exception vasp.automatedPostprocessing.postprocessing_h5py.chroma_filters.ParameterError[source]#

Exception class for mal-formed inputs

vasp.automatedPostprocessing.postprocessing_h5py.chroma_filters.chroma_filterbank(sr, n_fft, n_chroma=12, tuning=0.0, ctroct=5.0, octwidth=2, norm=2, base_c=True, dtype=<class 'numpy.float32'>)[source]#

Create a chroma filter bank.

This creates a linear transformation matrix to project FFT bins onto chroma bins (i.e. pitch classes).

Parameters:
  • sr (number > 0 [scalar]) – audio sampling rate

  • n_fft (int > 0 [scalar]) – number of FFT bins

  • n_chroma (int > 0 [scalar]) – number of chroma bins

  • tuning (float) – Tuning deviation from A440 in fractions of a chroma bin.

  • ctroct (float > 0 [scalar])

  • octwidth (float > 0 or None [scalar]) –

    ctroct and octwidth specify a dominance window: a Gaussian weighting centered on ctroct (in octs, A0 = 27.5Hz) and with a gaussian half-width of octwidth.

    Set octwidth to None to use a flat weighting.

  • norm (float > 0 or np.inf) – Normalization factor for each filter

  • base_c (bool) – If True, the filter bank will start at ‘C’. If False, the filter bank will start at ‘A’.

  • dtype (np.dtype) – The data type of the output basis. By default, uses 32-bit (single-precision) floating point.

Returns:

wts – Chroma filter matrix

Return type:

ndarray [shape=(n_chroma, 1 + n_fft / 2)]

See also

librosa.util.normalize, librosa.feature.chroma_stft

Notes

This function caches at level 10.

Examples

Build a simple chroma filter bank

>>> chromafb = librosa.filters.chroma(22050, 4096)
array([[  1.689e-05,   3.024e-04, ...,   4.639e-17,   5.327e-17],
       [  1.716e-05,   2.652e-04, ...,   2.674e-25,   3.176e-25],
...,
       [  1.578e-05,   3.619e-04, ...,   8.577e-06,   9.205e-06],
       [  1.643e-05,   3.355e-04, ...,   1.474e-10,   1.636e-10]])

Use quarter-tones instead of semitones

>>> librosa.filters.chroma(22050, 4096, n_chroma=24)
array([[  1.194e-05,   2.138e-04, ...,   6.297e-64,   1.115e-63],
       [  1.206e-05,   2.009e-04, ...,   1.546e-79,   2.929e-79],
...,
       [  1.162e-05,   2.372e-04, ...,   6.417e-38,   9.923e-38],
       [  1.180e-05,   2.260e-04, ...,   4.697e-50,   7.772e-50]])

Equally weight all octaves

>>> librosa.filters.chroma(22050, 4096, octwidth=None)
array([[  3.036e-01,   2.604e-01, ...,   2.445e-16,   2.809e-16],
       [  3.084e-01,   2.283e-01, ...,   1.409e-24,   1.675e-24],
...,
       [  2.836e-01,   3.116e-01, ...,   4.520e-05,   4.854e-05],
       [  2.953e-01,   2.888e-01, ...,   7.768e-10,   8.629e-10]])
>>> import matplotlib.pyplot as plt
>>> fig, ax = plt.subplots()
>>> img = librosa.display.specshow(chromafb, x_axis='linear', ax=ax)
>>> ax.set(ylabel='Chroma filter', title='Chroma filter bank')
>>> fig.colorbar(img, ax=ax)
vasp.automatedPostprocessing.postprocessing_h5py.chroma_filters.hz_to_octs(frequencies, tuning=0.0, bins_per_octave=12)[source]#

Convert frequencies (Hz) to (fractional) octave numbers.

Examples

>>> librosa.hz_to_octs(440.0)
4.
>>> librosa.hz_to_octs([32, 64, 128, 256])
array([ 0.219,  1.219,  2.219,  3.219])
Parameters:
  • frequencies (number >0 or np.ndarray [shape=(n,)] or float) – scalar or vector of frequencies

  • tuning (float) – Tuning deviation from A440 in (fractional) bins per octave.

  • bins_per_octave (int > 0) – Number of bins per octave.

Returns:

octaves – octave number for each frequency

Return type:

number or np.ndarray [shape=(n,)]

See also

octs_to_hz

vasp.automatedPostprocessing.postprocessing_h5py.chroma_filters.normalize(S, norm=inf, axis=0, threshold=None, fill=None)[source]#

Normalize an array along a chosen axis.

Given a norm (described below) and a target axis, the input array is scaled so that:

norm(S, axis=axis) == 1

For example, axis=0 normalizes each column of a 2-d array by aggregating over the rows (0-axis). Similarly, axis=1 normalizes each row of a 2-d array.

This function also supports thresholding small-norm slices: any slice (i.e., row or column) with norm below a specified threshold can be left un-normalized, set to all-zeros, or filled with uniform non-zero values that normalize to 1.

Note: the semantics of this function differ from scipy.linalg.norm in two ways: multi-dimensional arrays are supported, but matrix-norms are not.

Parameters:
  • S (np.ndarray) – The matrix to normalize

  • norm ({np.inf, -np.inf, 0, float > 0, None}) –

    • np.inf : maximum absolute value

    • -np.inf : mininum absolute value

    • 0 : number of non-zeros (the support)

    • floatcorresponding l_p norm

      See scipy.linalg.norm for details.

    • None : no normalization is performed

  • axis (int [scalar]) – Axis along which to compute the norm.

  • threshold (number > 0 [optional]) –

    Only the columns (or rows) with norm at least threshold are normalized.

    By default, the threshold is determined from the numerical precision of S.dtype.

  • fill (None or bool) –

    If None, then columns (or rows) with norm below threshold are left as is.

    If False, then columns (rows) with norm below threshold are set to 0.

    If True, then columns (rows) with norm below threshold are filled uniformly such that the corresponding norm is 1.

    Note

    fill=True is incompatible with norm=0 because no uniform vector exists with l0 “norm” equal to 1.

Returns:

S_norm – Normalized array

Return type:

np.ndarray [shape=S.shape]

Raises:

ParameterError – If norm is not among the valid types defined above If S is not finite If fill=True and norm=0

See also

scipy.linalg.norm

Notes

This function caches at level 40.

Examples

>>> # Construct an example matrix
>>> S = np.vander(np.arange(-2.0, 2.0))
>>> S
array([[-8.,  4., -2.,  1.],
       [-1.,  1., -1.,  1.],
       [ 0.,  0.,  0.,  1.],
       [ 1.,  1.,  1.,  1.]])
>>> # Max (l-infinity)-normalize the columns
>>> librosa.util.normalize(S)
array([[-1.   ,  1.   , -1.   ,  1.   ],
       [-0.125,  0.25 , -0.5  ,  1.   ],
       [ 0.   ,  0.   ,  0.   ,  1.   ],
       [ 0.125,  0.25 ,  0.5  ,  1.   ]])
>>> # Max (l-infinity)-normalize the rows
>>> librosa.util.normalize(S, axis=1)
array([[-1.   ,  0.5  , -0.25 ,  0.125],
       [-1.   ,  1.   , -1.   ,  1.   ],
       [ 0.   ,  0.   ,  0.   ,  1.   ],
       [ 1.   ,  1.   ,  1.   ,  1.   ]])
>>> # l1-normalize the columns
>>> librosa.util.normalize(S, norm=1)
array([[-0.8  ,  0.667, -0.5  ,  0.25 ],
       [-0.1  ,  0.167, -0.25 ,  0.25 ],
       [ 0.   ,  0.   ,  0.   ,  0.25 ],
       [ 0.1  ,  0.167,  0.25 ,  0.25 ]])
>>> # l2-normalize the columns
>>> librosa.util.normalize(S, norm=2)
array([[-0.985,  0.943, -0.816,  0.5  ],
       [-0.123,  0.236, -0.408,  0.5  ],
       [ 0.   ,  0.   ,  0.   ,  0.5  ],
       [ 0.123,  0.236,  0.408,  0.5  ]])
>>> # Thresholding and filling
>>> S[:, -1] = 1e-308
>>> S
array([[ -8.000e+000,   4.000e+000,  -2.000e+000,
          1.000e-308],
       [ -1.000e+000,   1.000e+000,  -1.000e+000,
          1.000e-308],
       [  0.000e+000,   0.000e+000,   0.000e+000,
          1.000e-308],
       [  1.000e+000,   1.000e+000,   1.000e+000,
          1.000e-308]])
>>> # By default, small-norm columns are left untouched
>>> librosa.util.normalize(S)
array([[ -1.000e+000,   1.000e+000,  -1.000e+000,
          1.000e-308],
       [ -1.250e-001,   2.500e-001,  -5.000e-001,
          1.000e-308],
       [  0.000e+000,   0.000e+000,   0.000e+000,
          1.000e-308],
       [  1.250e-001,   2.500e-001,   5.000e-001,
          1.000e-308]])
>>> # Small-norm columns can be zeroed out
>>> librosa.util.normalize(S, fill=False)
array([[-1.   ,  1.   , -1.   ,  0.   ],
       [-0.125,  0.25 , -0.5  ,  0.   ],
       [ 0.   ,  0.   ,  0.   ,  0.   ],
       [ 0.125,  0.25 ,  0.5  ,  0.   ]])
>>> # Or set to constant with unit-norm
>>> librosa.util.normalize(S, fill=True)
array([[-1.   ,  1.   , -1.   ,  1.   ],
       [-0.125,  0.25 , -0.5  ,  1.   ],
       [ 0.   ,  0.   ,  0.   ,  1.   ],
       [ 0.125,  0.25 ,  0.5  ,  1.   ]])
>>> # With an l1 norm instead of max-norm
>>> librosa.util.normalize(S, norm=1, fill=True)
array([[-0.8  ,  0.667, -0.5  ,  0.25 ],
       [-0.1  ,  0.167, -0.25 ,  0.25 ],
       [ 0.   ,  0.   ,  0.   ,  0.25 ],
       [ 0.1  ,  0.167,  0.25 ,  0.25 ]])
vasp.automatedPostprocessing.postprocessing_h5py.chroma_filters.octs_to_hz(octs, tuning=0.0, bins_per_octave=12)[source]#

Convert octaves numbers to frequencies.

Octaves are counted relative to A.

Examples

>>> librosa.octs_to_hz(1)
55.
>>> librosa.octs_to_hz([-2, -1, 0, 1, 2])
array([   6.875,   13.75 ,   27.5  ,   55.   ,  110.   ])
Parameters:
  • octaves (np.ndarray [shape=(n,)] or float) – octave number for each frequency

  • tuning (float) – Tuning deviation from A440 in (fractional) bins per octave.

  • bins_per_octave (int > 0) – Number of bins per octave.

Returns:

frequencies – scalar or vector of frequencies

Return type:

number or np.ndarray [shape=(n,)]

See also

hz_to_octs

vasp.automatedPostprocessing.postprocessing_h5py.chroma_filters.tiny(x)[source]#

Compute the tiny-value corresponding to an input’s data type.

This is the smallest “usable” number representable in x.dtype (e.g., float32).

This is primarily useful for determining a threshold for numerical underflow in division or multiplication operations.

Parameters:

x (number or np.ndarray) – The array to compute the tiny-value for. All that matters here is x.dtype

Returns:

tiny_value – The smallest positive usable number for the type of x. If x is integer-typed, then the tiny value for np.float32 is returned instead.

Return type:

float

See also

numpy.finfo

Examples

For a standard double-precision floating point number:

>>> librosa.util.tiny(1.0)
2.2250738585072014e-308

Or explicitly as double-precision

>>> librosa.util.tiny(np.asarray(1e-5, dtype=np.float64))
2.2250738585072014e-308

Or complex numbers

>>> librosa.util.tiny(1j)
2.2250738585072014e-308

Single-precision floating point:

>>> librosa.util.tiny(np.asarray(1e-5, dtype=np.float32))
1.1754944e-38

Integer

>>> librosa.util.tiny(5)
1.1754944e-38

This script creates spectrograms, power spectral density and chromagrams from formatted matrices (.npz files)”

vasp.automatedPostprocessing.postprocessing_h5py.create_spectrograms_chromagrams.create_spectrogram_composite(case_name: str, quantity: str, df: DataFrame, start_t: float, end_t: float, num_windows_per_sec: float, overlap_frac: float, window: str, lowcut: float, min_color: float, max_color: float, image_folder: str | Path, flow_rate_file: str | Path | None = None, amplitude_file: str | Path | None = None, power_scaled: bool = False, ylim: float | None = None) None[source]#

Create a composite spectrogram figure.

Parameters:
  • case_name (str) – Path to simulation results.

  • quantity (str) – Quantity to postprocess.

  • df (pd.DataFrame) – Input dataframe.

  • start_t (float) – Start time for analysis.

  • end_t (float) – End time for analysis.

  • num_windows_per_sec (float) – Number of windows per second.

  • overlap_frac (float) – Overlap fraction for windows.

  • window (str) – Type of window for spectrogram.

  • lowcut (float) – Lowcut frequency for high-pass filter.

  • min_color (float) – Minimum value for the color range.

  • max_color (float) – Maximum value for the color range.

  • image_folder (str or Path) – Folder to save the images.

  • flow_rate_file (str or Path, optional) – File containing flow rate data.

  • amplitude_file (str or Path, optional) – File containing amplitude data.

  • power_scaled (bool, optional) – Whether to scale the power.

  • ylim (float, optional) – Y-axis limit for the plot.

vasp.automatedPostprocessing.postprocessing_h5py.create_spectrograms_chromagrams.main()[source]#

This script creates a power spectrum plot.

vasp.automatedPostprocessing.postprocessing_h5py.create_spectrum.create_spectrum(case_name: str, quantity: str, df, start_t: float, end_t: float, num_windows_per_sec: float, overlap_frac: float, window: str, lowcut: float, min_color: float, max_color: float, image_folder: str | Path, flow_rate_file: str | None = None, amplitude_file: str | None = None, power_scaled: bool = False) None[source]#

Create a power spectrum plot and save the results as an image and CSV file.

Parameters:
  • case_name (str) – Name of the case.

  • quantity (str) – Type of data to be processed.

  • df – Input DataFrame containing relevant data.

  • start_t (float) – Desired start time of the output files.

  • end_t (float) – Desired end time of the output files.

  • num_windows_per_sec (float) – Number of windows per second.

  • overlap_frac (float) – Fraction of overlap between consecutive windows.

  • window (str) – Type of window function to use.

  • lowcut (float) – Cutoff frequency for the high-pass filter.

  • min_color (float) – Minimum value for the color range.

  • max_color (float) – Maximum value for the color range.

  • image_folder (str or Path) – Folder to save the spectrum image and CSV file.

  • flow_rate_file (str) – File name for flow rate data.

  • amplitude_file (str) – File name for amplitude data.

  • power_scaled (bool) – Whether to use power scaling in the PSD calculation.

Returns:

Saves the spectrum plot as an image and CSV file.

Return type:

None

vasp.automatedPostprocessing.postprocessing_h5py.create_spectrum.main()[source]#

This file contains helper functions for creating visualizations outside of FEniCS.

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.calculate_windowed_rms(signal_array: ndarray, window_size: int, window_type: str = 'flat') ndarray[source]#

Calculate the windowed root mean squared (RMS) amplitude of a signal.

Parameters:
  • signal_array (numpy.ndarray) – Input signal.

  • window_size (int) – Size of the window in number of timesteps.

  • window_type (str, optional) – Type of window function to use. Default is “flat”. Supported window types: “flat”, “tukey”, “hann”, “blackmanharris”, “flattop”.

Returns:

Windowed RMS amplitudes.

Return type:

numpy.ndarray

References

https://stackoverflow.com/questions/8245687/numpy-root-mean-squared-rms-smoothing-of-a-signal https://stackoverflow.com/questions/47484899/moving-average-produces-array-of-different-length

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.create_checkpoint_xdmf_file(num_ts: int, time_between_files: float, start_t: float, n_elements: int, n_nodes: int, att_type: str, viz_type: str, output_folder: Path) None[source]#

Create an XDMF file for a time series visualization. This function is specifically for the data genearted by FEniCS write_checkpoint function.

Parameters:
  • num_ts (int) – Number of time steps.

  • time_between_files (float) – Time interval between files.

  • start_t (float) – Starting time.

  • n_elements (int) – Number of elements.

  • n_nodes (int) – Number of nodes.

  • att_type (str) – Type of attribute - “Scalar”, “Vector”, or “Tensor”.

  • viz_type (str) – Visualization type.

  • output_folder (Path) – Path to the output folder.

Returns:

None

Raises:

ValueError – If an unsupported attribute type is provided.

Note

We assume that the function is discontinuous Galerkin and the element degree is 1.

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.create_point_trace(formatted_data_folder: str, output_folder: str, point_ids: List[int], time_between_files: float, start_t: float, dvp: str) None[source]#

Create point traces for specified point IDs and save the results in CSV and PNG files.

Parameters:
  • formatted_data_folder (str) – Path to the folder containing formatted data.

  • output_folder (str) – Path to the folder where output files will be saved.

  • point_ids (List[int]) – List of point IDs for which traces will be created.

  • time_between_files (float) – Time between files in seconds.

  • start_t (float) – Start time of the simulation.

  • dvp (str) – Type of visualization (‘v’ for velocity, ‘d’ for displacement, ‘p’ for pressure).

Returns:

None

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.create_transformed_matrix(input_path: str | Path, output_folder: str | Path, mesh_path: str | Path, case_name: str, start_t: float, end_t: float, quantity: str, fluid_domain_id: int | list[int], solid_domain_id: int | list[int], stride: int = 1) Tuple[float, dict[str, ndarray] | None, dict[str, ndarray] | None][source]#

Create a transformed matrix from simulation data.

Parameters:
  • input_path (str or Path) – Path to the input simulation data.

  • output_folder (str or Path) – Path to the output folder where the transformed matrix will be stored.

  • mesh_path (str or Path) – Path to the input mesh data.

  • case_name (str) – Name of the simulation case.

  • start_t (float) – Start time for extracting data.

  • end_t (float) – End time for extracting data.

  • quantity (str) – Quantity to extract (e.g., ‘d’ for displacement, ‘v’ for velocity).

  • fluid_domain_id (int or list) – ID of the fluid domain

  • solid_domain_id (int or list) – ID of the solid domain

  • stride (int) – Stride for selecting timesteps.

Returns:

A tuple containing the time between files, dof_info_dict,

Return type:

Tuple[float, dict[str, np.ndarray], dict[str, np.ndarray]]

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.create_xdmf_file(num_ts: int, time_between_files: float, start_t: float, n_elements: int, n_nodes: int, att_type: str, viz_type: str, output_folder: Path) None[source]#

Create an XDMF file for a time series visualization.

Parameters:
  • num_ts (int) – Number of time steps.

  • time_between_files (float) – Time interval between files.

  • start_t (float) – Starting time.

  • n_elements (int) – Number of elements.

  • n_nodes (int) – Number of nodes.

  • att_type (str) – Type of attribute - “Scalar”, “Vector”, or “Tensor”.

  • viz_type (str) – Visualization type.

  • output_folder (Path) – Path to the output folder.

Returns:

None

Raises:

ValueError – If an unsupported attribute type is provided.

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.get_coords(mesh_path: str | Path) ndarray[source]#

Get coordinates from a mesh file.

Parameters:

mesh_path (str or Path) – Path to the mesh file.

Returns:

Array containing the coordinates.

Return type:

np.ndarray

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.get_domain_ids_specified_region(mesh_path: str | Path, fluid_sampling_domain_id: int, solid_sampling_domain_id: int) Tuple[ndarray, ndarray, ndarray][source]#

Obtain node IDs for the fluid, solid, and all elements within specified regions of the input mesh.

Parameters:
  • mesh_path (str or Path) – The file path of the input mesh.

  • fluid_sampling_domain_id (int) – Domain ID for the fluid region to be sampled.

  • solid_sampling_domain_id (int) – Domain ID for the solid region to be sampled.

Returns:

Node IDs for fluid, solid, and all elements.

Return type:

Tuple[np.ndarray, np.ndarray, np.ndarray]

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.get_eig(T: ndarray) float[source]#

Analytically calculate eigenvalues for a three-dimensional tensor T with a characteristic polynomial equation of the form

lambda^3 - I1*lambda^2 + I2*lambda - I3 = 0 .

Since the characteristic polynomial is in its normal form , the eigenvalues can be determined using Cardanos formula. This algorithm is based on: “Efficient numerical diagonalization of hermitian 3 by 3 matrices” by J.Kopp, eqn 21-34, with coefficients: c2=-I1, c1 = I2, c3 = -I3).

NOTE: The method implemented here, implicitly assumes that the polynomial has only real roots, since imaginary ones should not occur in this use case.

In order to ensure eigenvalues with algebraic multiplicity of 1, the idea of numerical perturbations is adopted from “Computation of isotropic tensor functions” by C. Miehe (1993). Since direct comparisons with conditionals have proven to be very slow, not the eigenvalues but the coefficients occuring during the calculation of them are perturbated to get distinct values.

Parameters:

T (np.ndarray) – Three-dimensional tensor.

Returns:

First eigenvalue.

Return type:

float

References

https://fenicsproject.discourse.group/t/hyperelastic-model-problems-on-plotting-stresses/3130/6

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.get_interface_ids(mesh_path: str | Path, fluid_domain_id: int | list[int], solid_domain_id: int | list[int]) ndarray[source]#

Get the interface node ID’s between fluid and solid domains from the given mesh file.

Parameters:
  • mesh_path (str or Path) – Path to the mesh file.

  • fluid_domain_id (int or list) – ID of the fluid domain

  • solid_domain_id (int or list) – ID of the solid domain

Returns:

Array containing the interface node IDs.

Return type:

np.ndarray

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.get_sampling_constants(df: DataFrame, start_t: float, end_t: float) Tuple[float, int, float][source]#

Calculate sampling constants from a DataFrame.

Parameters:
  • df (DataFrame) – The input DataFrame.

  • start_t (float) – The start time of the data.

  • end_t (float) – The end time of the data.

Returns:

A tuple containing the period (T), number of samples per cycle (nsamples), and sample rate (fs).

Return type:

Tuple[float, int, float]

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.get_surface_topology_coords(out_file: str | Path) tuple[source]#

Get surface topology and coordinates from an output file.

Parameters:

out_file (str or Path) – Path to the output file.

Returns:

Tuple containing the surface topology and coordinates.

Return type:

tuple

vasp.automatedPostprocessing.postprocessing_h5py.postprocessing_common_h5py.read_npz_files(filepath: str | Path) DataFrame[source]#

Read data from an npz file and return it as a DataFrame.

Parameters:

filepath (str or Path) – Path to the npz file.

Returns:

DataFrame containing the data.

Return type:

pd.DataFrame

This file contains helper functions for creating spectrograms.

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.butter_bandpass(lowcut: float, highcut: float, fs: float, order: int = 5, btype: str = 'band') tuple[source]#

Design a Butterworth bandpass, bandstop, highpass, or lowpass filter.

Parameters:
  • lowcut (float) – Cutoff frequency for low cut.

  • highcut (float) – Cutoff frequency for high cut (ignored if btype is ‘highpass’).

  • fs (float) – Sampling frequency in samples per second.

  • order (int, optional) – Order of the filter. Default is 5.

  • btype (str, optional) – Type of filter (‘band’, ‘stop’, ‘highpass’, ‘lowpass’, or ‘bandpass’). Default is ‘band’.

Returns:

Numerator (b) and denominator (a) coefficients of the filter.

Return type:

tuple

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.butter_bandpass_filter(data: ndarray, lowcut: float = 25.0, highcut: float = 15000.0, fs: float = 2500.0, order: int = 5, btype: str = 'band') ndarray[source]#

Apply a Butterworth bandpass, bandstop, highpass, or lowpass filter to the input data.

Parameters:
  • data (np.ndarray) – Input data to filter.

  • lowcut (float, optional) – Low cutoff frequency. Default is 25.0.

  • highcut (float, optional) – High cutoff frequency. Default is 15000.0.

  • fs (float, optional) – Sampling frequency. Default is 2500.0.

  • order (int, optional) – Order of the filter. Default is 5.

  • btype (str, optional) – Type of filter (‘band’, ‘stop’, ‘highpass’, ‘lowpass’). Default is ‘band’.

Returns:

Filtered data.

Return type:

np.ndarray

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.calc_chroma_entropy(chroma: ndarray, n_chroma: int) ndarray[source]#

Calculate chroma entropy.

Parameters:
  • chroma (np.ndarray) – Chromagram.

  • n_chroma (int) – Number of chroma bins.

Returns:

Chroma entropy.

Return type:

np.ndarray

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.chromagram_from_spectrogram(Pxx: ndarray, fs: float, n_fft: int, n_chroma: int = 24, norm: bool | str = True) ndarray[source]#

Calculate chromagram from a spectrogram.

Parameters:
  • Pxx (np.ndarray) – Input spectrogram.

  • fs (float) – Sampling frequency.

  • n_fft (int) – Number of FFT points.

  • n_chroma (int, optional) – Number of chroma bins. Default is 24.

  • norm (bool, optional) – Normalize chroma. Options are ‘max’, ‘sum’, or False for no normalization. Default is True.

Returns:

Chromagram.

Return type:

np.ndarray

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.compute_average_spectrogram(df: DataFrame, fs: float, nWindow: int, overlapFrac: float, window: str, start_t: float, end_t: float, thresh: float, scaling: str = 'spectrum', filter_data: bool = False, thresh_method: str = 'new') tuple[source]#

Compute the average spectrogram for a DataFrame of time series data.

Parameters:
  • df (pd.DataFrame) – Input DataFrame containing time series data.

  • fs (float) – Sampling frequency.

  • nWindow (int) – Number of samples per window.

  • overlapFrac (float) – Fraction of overlap between windows.

  • window (str) – Window function for spectrogram.

  • start_t (float) – Start time for the spectrogram.

  • end_t (float) – End time for the spectrogram.

  • thresh (float) – Threshold value for scaling.

  • scaling (str, optional) – Scaling for the spectrogram (‘density’ or ‘spectrum’). Default is ‘spectrum’.

  • filter_data (bool, optional) – Apply a Butterworth highpass filter to the data. Default is False.

  • thresh_method (str, optional) – Method for thresholding (‘old’, ‘log_only’, ‘new’). Default is ‘new’.

Returns:

Time bins (bins), frequency values (freqs), scaled Power Spectral Density matrix (Pxx_scaled),

maximum value after scaling (max_val), minimum value after scaling (min_val), and the lower threshold used for scaling.

Return type:

tuple

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.filter_time_data(df: DataFrame, fs: float, lowcut: float = 25.0, highcut: float = 15000.0, order: int = 6, btype: str = 'highpass') DataFrame[source]#

Apply a Butterworth highpass, lowpass, bandpass, or bandstop filter to the time series data in a DataFrame.

Parameters:
  • df (pd.DataFrame) – Input DataFrame containing time series data.

  • fs (float) – Sampling frequency.

  • lowcut (float, optional) – Low cutoff frequency. Default is 25.0.

  • highcut (float, optional) – High cutoff frequency. Default is 15000.0.

  • order (int, optional) – Order of the filter. Default is 6.

  • btype (str, optional) – Type of filter (‘highpass’, ‘lowpass’, ‘bandpass’, ‘bandstop’). Default is ‘highpass’.

Returns:

DataFrame containing filtered time series data.

Return type:

pd.DataFrame

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.find_points_in_box(x_min: float, x_max: float, y_min: float, y_max: float, z_min: float, z_max: float, coords: ndarray) ndarray[source]#

Find points within a box defined by its minimum and maximum x, y, and z coordinates.

Parameters:
  • x_min (float) – Minimum x coordinate of the box.

  • x_max (float) – Maximum x coordinate of the box.

  • y_min (float) – Minimum y coordinate of the box.

  • y_max (float) – Maximum y coordinate of the box.

  • z_min (float) – Minimum z coordinate of the box.

  • z_max (float) – Maximum z coordinate of the box.

  • coords (np.ndarray) – The coordinates of mesh nodes as a 2D NumPy array with shape (n, 3).

Returns:

Indices of points within the box.

Return type:

np.ndarray

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.find_points_in_sphere(center: ndarray, radius: float, coords: ndarray) ndarray[source]#

Find points within a sphere defined by its center and radius.

Parameters:
  • center (np.ndarray) – The center of the sphere as a 1D NumPy array with shape (3,).

  • radius (float) – The radius of the sphere.

  • coords (np.ndarray) – The coordinates of mesh nodes as a 2D NumPy array with shape (n, 3).

Returns:

Indices of points within the sphere.

Return type:

np.ndarray

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.get_psd(dfNearest: DataFrame, fsamp: float, scaling: str = 'density') tuple[source]#

Calculate the Power Spectral Density (PSD) of a DataFrame of signals.

Parameters:
  • dfNearest (pd.DataFrame) – DataFrame containing signals in rows.

  • fsamp (float) – Sampling frequency of the signals.

  • scaling (str, optional) – Scaling applied to the PSD. Default is “density”.

Returns:

A tuple containing the mean PSD matrix and the corresponding frequency values.

Return type:

tuple

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.get_sampling_constants(df: DataFrame, start_t: float, end_t: float) tuple[source]#

Get sampling constants such as period, number of samples, and sample rate.

Parameters:
  • df (pd.DataFrame) – Input DataFrame containing time series data.

  • start_t (float) – Start time of the data.

  • end_t (float) – End time of the data.

Returns:

Period, number of samples, and sample rate.

Return type:

tuple

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.get_spectrogram(dfNearest: DataFrame, fsamp: float, nWindow: int, overlapFrac: float, window: str, start_t: float, end_t: float, scaling: str = 'spectrum', interpolate: bool = False) tuple[source]#

Calculates spectrogram.

Parameters:
  • dfNearest (pd.DataFrame) – DataFrame of shape (num_points, num_timesteps).

  • fsamp (float) – Sampling frequency.

  • nWindow (int) – Number of samples per window.

  • overlapFrac (float) – Fraction of overlap between windows.

  • window (str) – Window function for spectrogram.

  • start_t (float) – Start time for the spectrogram.

  • end_t (float) – End time for the spectrogram.

  • scaling (str, optional) – Scaling for the spectrogram (‘density’ or ‘spectrum’). Default is ‘spectrum’.

  • interpolate (bool, optional) – Perform interpolation. Default is False.

Returns:

Power Spectral Density matrix (Pxx_mean), frequency values (freqs), and time bins (bins).

Return type:

tuple

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.plot_chromagram(fig1: Figure, ax1: Axes, bins: ndarray, chroma: ndarray, title: str | None = None, path: str | Path | None = None, convert_a: float = 1.0, convert_b: float = 0.0, x_label: str | None = None, shading: Literal['flat', 'nearest', 'gouraud', 'auto'] | None = 'gouraud', color_range: list[float] | None = None) None[source]#

Plot a chromagram.

Parameters:
  • fig1 (plt.Figure) – Matplotlib figure to plot on.

  • ax1 (plt.Axes) – Matplotlib axes to plot on.

  • bins (np.ndarray) – Time bins.

  • chroma (np.ndarray) – Chromagram values.

  • title (str, optional) – Title of the plot. Default is None.

  • path (str, optional) – Path to save the figure. Default is None.

  • convert_a (float, optional) – Conversion factor for the x-axis. Default is 1.0.

  • convert_b (float, optional) – Offset for the x-axis conversion. Default is 0.0.

  • x_label (str, optional) – Label for the x-axis. Default is None.

  • shading (str, optional) – Shading style for the plot. Default is ‘gouraud’.

  • color_range (list[float], optional) – Range for the color scale. Default is None.

Returns:

None

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.plot_spectrogram(fig1: Figure, ax1: Axes, bins: ndarray, freqs: ndarray, Pxx: ndarray, ylim: float | None = None, title: str | None = None, convert_a: float = 0.0, convert_b: float = 0.0, x_label: str | None = None, color_range: list[float] | None = None) None[source]#

Plot a spectrogram.

Parameters:
  • fig1 (plt.Figure) – Matplotlib figure to plot on.

  • ax1 (plt.Axes) – Matplotlib axes to plot on.

  • bins (np.ndarray) – Time bins.

  • freqs (np.ndarray) – Frequency values.

  • Pxx (np.ndarray) – Power spectral density values.

  • ylim (float, optional) – Maximum frequency to display on the y-axis.

  • title (str, optional) – Title of the plot. Default is None.

  • convert_a (float, optional) – Conversion factor for the x-axis. Default is 0.0.

  • convert_b (float, optional) – Offset for the x-axis conversion. Default is 0.0.

  • x_label (str, optional) – Label for the x-axis. Default is None.

  • color_range (list[float], optional) – Range for the color scale. Default is None.

Returns:

None

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.read_command_line_spec() Namespace[source]#

Read arguments from the command line using ConfigArgParse.

Returns:

Parsed command-line arguments.

Return type:

Namespace

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.read_spectrogram_data(folder: str | Path, mesh_path: str | Path, save_deg: int, stride: int, start_t: float, end_t: float, n_samples: int, sampling_region: str, fluid_sampling_domain_id: int, solid_sampling_domain_id: int, fsi_region: list[float], quantity: str, interface_only: bool, component: str, point_ids: list[int], fluid_domain_id: int | list[int], solid_domain_id: int | list[int], sampling_method: str = 'RandomPoint')[source]#

Read spectrogram data and perform processing steps.

Parameters:
  • folder (str or Path) – Path to simulation results.

  • mesh_path (str or Path) – Path to the mesh file.

  • save_deg (int) – Degree of mesh refinement.

  • stride (int) – Desired frequency of output data.

  • start_t (float) – Start time for data processing.

  • end_t (float) – End time for data processing.

  • n_samples (int) – Number of samples.

  • sampling_region (str) – Region for sampling data (“sphere”, “domain” or “box”).

  • fluid_sampling_domain_id (int) – Domain ID for fluid sampling (used when sampling_region=”domain”).

  • solid_sampling_domain_id (int) – Domain ID for solid sampling (used when sampling_region=”domain”).

  • fsi_region (list) – x, y, and z coordinates of sphere center and radius of the sphere (used when sampling_region=”sphere”). In case of sampling_region=”box”, the list should contain [x_min, x_max, y_min, y_max, z_min, z_max]. The box is defined by the minimum and maximum values of x, y, and z.

  • quantity (str) – Quantity to postprocess.

  • interface_only (bool) – Whether to include only interface ID’s.

  • component (str) – Component of the data to be visualized.

  • point_ids (int) – List of Point IDs (used when sampling_method=”PointList”).

  • sampling_method (str) – Method for sampling data (“RandomPoint”, “PointList”, or “Spatial”).

  • fluid_domain_id (int or list) – ID of the fluid domain

  • solid_domain_id (int or list) – ID of the solid domain

Returns:

(Processed data type, DataFrame, Case name, Image folder, Hi-pass visualization folder).

Return type:

tuple

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.shift_bit_length(x: int) int[source]#

Round up to the nearest power of 2.

Parameters:

x (int) – Input integer.

Returns:

The smallest power of 2 greater than or equal to the input.

Return type:

int

Author:

Daniel Macdonald

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.sonify_point(case_name: str, quantity: str, df, start_t: float, end_t: float, overlap_frac: float, lowcut: float, image_folder: str) None[source]#

Sonify a point in the dataframe and save the resulting audio as a WAV file.

Parameters:
  • case_name (str) – Name of the case.

  • quantity (str) – Type of data to be sonified.

  • df (pd.DataFrame) – Input DataFrame containing relevant data.

  • start_t (float) – Start time for sonification.

  • end_t (float) – End time for sonification.

  • overlap_frac (float) – Fraction of overlap between consecutive segments.

  • lowcut (float) – Cutoff frequency for the high-pass filter.

  • image_folder (str) – Folder to save the sonified audio file.

Returns:

Saves the sonified audio file in WAV format.

Return type:

None

vasp.automatedPostprocessing.postprocessing_h5py.spectrograms.spectrogram_scaling(Pxx_mean: ndarray, lower_thresh: float) tuple[source]#

Scale a spectrogram.

Parameters:
  • Pxx_mean (np.ndarray) – Power Spectral Density matrix.

  • lower_thresh (float) – Threshold value for scaling.

Returns:

Scaled Power Spectral Density matrix (Pxx_scaled), maximum value after scaling (max_val),

minimum value after scaling (min_val), and the lower threshold used for scaling.

Return type:

tuple

Author:

Daniel Macdonald

common functions for postprocessing-mesh scripts

vasp.automatedPostprocessing.postprocessing_mesh.postprocessing_mesh_common.parse_arguments() Namespace[source]#

Parse command line arguments.

Returns:

Parsed command-line arguments.

Return type:

argparse.Namespace

vasp.automatedPostprocessing.postprocessing_mesh.separate_mesh.main() None[source]#
vasp.automatedPostprocessing.postprocessing_mesh.separate_mesh.separate_mesh(mesh_path: Path, fluid_domain_id: int | list, solid_domain_id: int | list, view: bool = False) None[source]#

Given a mesh file that contains fluid and solid domains, this function separates the domains and saves them as separate mesh files. These domain specific mesh files are later used in the other postprocessing scripts.

Parameters:
  • mesh_path (Path) – Path to the mesh file.

  • fluid_domain_id (int or list) – Domain ID for fluid domain.

  • solid_domain_id (int or list) – Domain ID for solid domain.

Returns:

None

This script creates a refined mesh with domain markers from a specified mesh. However, the node numbering may not be the same as the output file with save_deg = 2, so the node numbering is corrected to match the output files. Currently, it only runs in serial (not parallel) due to the “adapt” function used in fenics. This mesh is later used in the “postprocessing_h5” and “postprocessing_fenics” scripts.

vasp.automatedPostprocessing.postprocessing_mesh.create_refined_mesh.create_refined_mesh(folder_path: Path, mesh_path: Path) None[source]#
Parameters:
  • folder_path (Path) – Path to the simulation results folder.

  • mesh_path (Path) – Path to the mesh file.

Returns:

None

vasp.automatedPostprocessing.postprocessing_mesh.create_refined_mesh.main() None[source]#

FSI problem scripts#

Problem file for tiny cylinder FSI simulation

class vasp.simulations.cylinder.InnerP(t, t_ramp, P_final, **kwargs)[source]#
eval(value, x)[source]#
update(t)[source]#
value_shape()[source]#
class vasp.simulations.cylinder.VelInPara(t, t_ramp, v_max_final, n, dsi, mesh, **kwargs)[source]#
eval(value, x)[source]#
update(t)[source]#
value_shape()[source]#
vasp.simulations.cylinder.create_bcs(DVP, mesh, boundaries, P_final, v_max_final, fsi_id, inlet_id, inlet_outlet_s_id, rigid_id, psi, F_solid_linear, **namespace)[source]#
vasp.simulations.cylinder.get_mesh_domain_and_boundaries(mesh_path, **namespace)[source]#
vasp.simulations.cylinder.post_solve(dvp_, dt, mesh, inlet_area, mu_f, rho_f, n, dsi, **namespace)[source]#
vasp.simulations.cylinder.pre_solve(t, u_inflow_exp, p_out_bc_val, **namespace)[source]#
vasp.simulations.cylinder.set_problem_parameters(default_variables, **namespace)[source]#

Problem file for offset stenosis FSI simulation

class vasp.simulations.offset_stenosis.InnerP(t, t_ramp, An, Bn, period, P_mean, **kwargs)[source]#
eval(value, x)[source]#
update(t)[source]#
value_shape()[source]#
vasp.simulations.offset_stenosis.create_bcs(t, DVP, mesh, boundaries, mu_f, fsi_id, inlet_id, inlet_outlet_s_id, rigid_id, psi, F_solid_linear, p_deg, FC_file, Q_mean, P_FC_File, P_mean, T_Cycle, **namespace)[source]#
vasp.simulations.offset_stenosis.get_mesh_domain_and_boundaries(mesh_path, fsi_region, dx_f_id, fsi_id, rigid_id, outer_id, **namespace)[source]#
vasp.simulations.offset_stenosis.initiate(mesh_path, **namespace)[source]#
vasp.simulations.offset_stenosis.post_solve(probe_points, solid_probe_points, dvp_, dt, mesh, inlet_area, dsi, mu_f, rho_f, n, **namespace)[source]#
vasp.simulations.offset_stenosis.pre_solve(t, inlet, p_out_bc_val, **namespace)[source]#
vasp.simulations.offset_stenosis.set_problem_parameters(default_variables, **namespace)[source]#

Problem file for aneurysm FSI simulation

class vasp.simulations.aneurysm.InnerP(t, t_ramp, An, Bn, period, P_mean, **kwargs)[source]#
eval(value, x)[source]#
update(t)[source]#
value_shape()[source]#
vasp.simulations.aneurysm.create_bcs(t, DVP, mesh, boundaries, mu_f, fsi_id, inlet_id, inlet_outlet_s_id, rigid_id, psi, F_solid_linear, p_deg, FC_file, Q_mean, P_FC_File, P_mean, T_Cycle, **namespace)[source]#
vasp.simulations.aneurysm.get_mesh_domain_and_boundaries(mesh_path, fsi_region, fsi_id, rigid_id, outer_id, **namespace)[source]#
vasp.simulations.aneurysm.initiate(mesh_path, scale_probe, **namespace)[source]#
vasp.simulations.aneurysm.post_solve(dvp_, n, dsi, dt, mesh, inlet_area, mu_f, rho_f, probe_points, **namespace)[source]#
vasp.simulations.aneurysm.pre_solve(t, inlet, p_out_bc_val, **namespace)[source]#
vasp.simulations.aneurysm.set_problem_parameters(default_variables, **namespace)[source]#

Problem file for AVF FSI simulation

class vasp.simulations.avf.InnerP(t, dt, p_t_ramp_start, p_t_ramp_end, interp_P, **kwargs)[source]#
eval(value, x)[source]#
update(t)[source]#
value_shape()[source]#
class vasp.simulations.avf.VelInPara(t, dt, vel_t_ramp, n, dsi, mesh, interp_velocity, **kwargs)[source]#
eval(value, x)[source]#
update(t)[source]#
value_shape()[source]#
vasp.simulations.avf.create_bcs(DVP, mesh, boundaries, T, dt, fsi_id, inlet_id1, inlet_id2, rigid_id, psi, F_solid_linear, vel_t_ramp, p_t_ramp_start, p_t_ramp_end, p_deg, v_deg, patient_data_path, **namespace)[source]#
vasp.simulations.avf.get_mesh_domain_and_boundaries(mesh_path, fsi_region, fsi_id, rigid_id, outer_id, **namespace)[source]#
vasp.simulations.avf.initiate(mesh_path, scale_probe, **namespace)[source]#
vasp.simulations.avf.post_solve(dvp_, n, dsi1, dt, mesh, inlet_area, mu_f, rho_f, probe_points, **namespace)[source]#
vasp.simulations.avf.pre_solve(t, u_inflow_exp1, u_inflow_exp2, p_out_bc_val, **namespace)[source]#
vasp.simulations.avf.set_problem_parameters(default_variables, **namespace)[source]#