Unlocking Structural Stability: Buckling Analysis with Code_Aster

Published by Ruggero Poletto on


Structural stability is paramount in design. While static analysis helps us understand stress and deformation, it doesn’t always tell the whole story. A slender column, perfectly safe under a static load, can suddenly collapse due to buckling when that load reaches a critical point. This phenomenon is a catastrophic failure mode, and accurately predicting it is where Code_Aster truly shines.

In this blog post, we’ll dive into how to perform a linear buckling analysis using Code_Aster, focusing on the essential commands in your .comm (command) file and how to interpret the results.

Why Code_Aster for Buckling?

Code_Aster is an incredibly powerful open-source finite element solver developed by EDF (Électricité de France). It’s renowned for its robust capabilities, especially in non-linear and stability analyses. Its command file system, while initially steep in its learning curve, offers unparalleled flexibility and control over your simulation.

The .comm File: Your Simulation Blueprint

The .comm file is the heart of any Code_Aster analysis. It’s a Python-like script that orchestrates the entire simulation, from defining material properties to running the solver and exporting results. For buckling analysis, we’ll primarily leverage two key operators: CALC_ELEM (or ASSE_MODELE / ASSE_MATRICE) to form the stiffness matrix, and crucially, MODE_MECA_SOLVEUR for the buckling Eigenvalue problem.

Let’s break down the typical structure for a linear buckling analysis:

1. Initialization and Mesh Reading

Every .comm file starts with basic setup.

Python

DEBUT()

# Read the mesh from a .med file (created in Salome or another preprocessor)
mail = LIRE_MAILLAGE(
    UNITE=20,
    FORMAT='MED'
)

This sets up the environment and imports your mesh.

2. Defining Model and Material Properties

Next, we define the finite element model and assign material properties.

Python

# Define the 3D Mechanical Model
modele = AFFE_MODELE(
    MAILLAGE=mail,
    AFFE=(
        _F(GROUP_MA=( 'my_volume' ), # Assign to a volume group in your mesh
           PHENOMENE='MECANIQUE',
           MODELISATION='3D',
           FORMULATION='ELAS'),
    )
)

# Define material properties (e.g., Steel)
materiau = DEFI_MATERIAU(
    ELAS=(
        _F(E=2.1E11,     # Young's Modulus in Pa
           NU=0.3),      # Poisson's Ratio
    )
)

# Assign material to the model
model = AFFE_MATERIAU(
    MAILLAGE=mail,
    MODELE=modele,
    AFFE=_F(
        GROUP_MA=('my_volume',),
        MATER=(materiau,),
    )
)

Here, AFFE_MODEL defines the type of analysis (3D mechanical, elastic formulation). DEFI_MATERIAU sets Young’s Modulus (E) and Poisson’s Ratio (NU), and AFFE_MATERIAU links it to your geometry.

3. Defining Boundary Conditions and Loads

This is where you constrain your model and apply the pre-buckling load. For buckling analysis, this is typically a static, “reference” load.

Python

# Define Fixed Boundary Conditions (e.g., fixing a face)
lacs = AFFE_CHAR_MECA(
    MODELE=modele,
    DDL_IMPO=(
        _F(GROUP_NO=('fixed_face_nodes',), # A node group on your fixed face
           DX=0.0, DY=0.0, DZ=0.0),
    )
)

# Define the reference load (e.g., a compressive force on a face)
force = AFFE_CHAR_MECA(
    MODELE=modele,
    FORCE_NODALE=(
        _F(GROUP_NO=('loaded_face_nodes',), # A node group on your loaded face
           FZ=-1.0E3), # A reference load (e.g., -1000 N in Z direction)
    )
)

DDL_IMPO applies prescribed displacements (fixed in this case), and FORCE_NODALE applies nodal forces. Remember, the magnitude of this load is arbitrary; the buckling analysis will give you a load multiplier.

4. Solving the Reference Static Analysis

Before buckling, we need to perform a static analysis to get the initial stress state. This is often handled by MECANIQUE which calls other functions like ASSE_MODELE and FACTORISATION.

Python

# Perform a static analysis with the reference load
res_statique = MECA_STATIQUE(
    MODELE=modele,
    CHAM_MATER=model,
    EXCIT=_F(CHARGE=force),
    LIAISON=lacs,
    # Other parameters can be added for output of static results
)

res_statique will contain the initial displacements and stresses.

5. The Buckling Analysis: MODE_MECA_SOLVEUR

This is the core function for buckling. It performs an eigenvalue analysis on the tangent stiffness matrix, accounting for the pre-stress state from the static analysis.

Python

# Perform the buckling analysis
resultat_buckling = MODE_MECA_SOLVEUR(
    MODELE=modele,
    CHAM_MATER=model,
    # Initial stress field from the static analysis
    CALC_PSEUDO_MODAL=_F(
        CHARGE_REF=(
            _F(CHARGE=force,),
        ),
        # Initial displacement field is taken from the static analysis results
        DEPL=res_statique.CHAM_NODA.DEPL,
    ),
    OPTION='PLUS_PETITE', # Look for the smallest eigenvalues (critical modes)
    NB_MODE=5,             # Request the first 5 buckling modes
)
  • CALC_PSEUDO_MODAL: This is where the magic happens. It tells Code_Aster to calculate the initial stress state due to the CHARGE_REF (our reference load) and use the DEPL field from the static analysis.
  • OPTION='PLUS_PETITE': We’re interested in the smallest eigenvalues, as these correspond to the lowest critical buckling loads.
  • NB_MODE: Specifies how many buckling modes (eigenvalues and eigenvectors) to extract.

6. Post-Processing and Output

Finally, we save the results in a format that can be visualized in a post-processor like ParaView.

Python

# Output results for post-processing
IMPR_RESU(
    RESU=_F(
        MAILLAGE=mail,
        RESULTAT=resultat_buckling,
        NOM_CHAM='DEPL_BUCK', # Name for displacement field of buckling modes
    ),
    FORMAT='MED',
    UNITE=80,
)

FIN()

IMPR_RESU writes the results to a .med file (UNIT=80) which you can then open in ParaView or Salome-Meca’s Post-Pro module.

Interpreting the Results

After running the .comm file, you’ll get several crucial pieces of information:

  1. Eigenvalues (Buckling Factors): These are the most important output. Each eigenvalue represents a load multiplier. If your reference load was P_ref, and Code_Aster returns an eigenvalue λ_i, then the critical buckling load for that mode is P_crit_i = λ_i * P_ref. The smallest positive eigenvalue is typically the most critical one, indicating the load at which your structure is most likely to buckle first.
  2. Eigenvectors (Buckling Mode Shapes): For each eigenvalue, there’s a corresponding eigenvector which describes the shape the structure takes when it buckles. Visualizing these mode shapes in ParaView is essential to understand how the structure will deform under buckling.

Example Interpretation:

If you applied a reference load of -1000N and Code_Aster returns an eigenvalue of 5.3 for the first mode:

  • Critical Buckling Load: 5.3 * 1000N = 5300N. This means your structure is predicted to buckle when the compressive load reaches 5300N.
  • Mode Shape: By visualizing the first mode, you might see a classic “bowing” of a column or a localized panel instability, giving you insight into where to reinforce your design.

Conclusion

Buckling analysis with Code_Aster is a powerful tool for ensuring the stability and safety of your designs. By carefully constructing your .comm file and understanding the output from MODE_MECA_SOLVEUR, you can accurately predict critical buckling loads and identify failure modes. While the initial learning curve for Code_Aster can be steep, the depth and flexibility it offers are incredibly rewarding for any serious CAE professional.

Have you used Code_Aster for buckling analysis? Share your experiences and tips in the comments below!


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Categories: Code Aster