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📁 C 开发的有限元软件
💻 FE
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fe assembleassemble ( )assemble (M, C)    Computes and returns the global stiffness matrix by computing the local    stiffness matrices and assembling them into the global matrix.  For    transient problems, if M is specified then it will contain the global    mass matrix on return.  Similarly, C will contain the global damping    matrix.  All matrices are compact.fe clear_nodesclear_nodes ( )    Clears the displacements and equivalent nodal force vectors for all    nodes in the current problem.fe compute_modescompute_modes (K, M)compute_modes (K, M, X)    Compute the modes for the given stiffness matrix, K, and mass matrix, M.    The result is the vector of eigenvalues.  If X is specified then it will    contain the matrix of eigenvectors upon return.fe compute_stressescompute_stresses (e)    Not available yet.fe construct_forcesconstruct_forces ( )construct_forces (t)    Constructs and returns the global nodal force vector based on all nodal    forces and the global DOFs active at those nodes.  For transient    problems, t may be a scalar expression used to specify the current time.    If t is missing then it is assumed to be zero.fe find_dofsfind_dofs ( )    Computes the set of active DOFs for the current problem.  As a result,    the DOF-related fields of the problem structure are initialized.  The    number of active DOFs is returned.fe global_dofglobal_dof (n, d)    Returns the global DOF corresponding to a local DOF.  The local DOF is    specified by its node, n, and the DOF, d.  The node may be specified as    either a node object or a node number.fe integrate_hyperbolicintegrate_hyperbolic (K, M, C)integrate_hyperbolic (K, M, C, p)    Solves the discrete equation of motion, Ma + Cv + Kd = F, using    Newmark's method with the Hilbert-Hughes-Taylor alpha correction for    improved accuracy with numerical damping.  The result is a matrix of    nodal displacements, with each column corresponding to a single time    step.  If the nodes have been renumbered then p should be used to    specify the permutation vector.  The sizes of the matrices must be    consistent with the definition of the problem.  Compact matrices are    expected.fe integrate_parabolicintegrate_parabolic (K, M)integrate_parabolic (K, M, p)    Solves the discrete parabolic differential equation Mv + Kd = F using a    generalized trapezoidal method.  If the nodes have been renumbered then    p should be used to specify the permutation vector.  The sizes of the    matrices must be consistent with the definition of the problem.  Compact    matrices are expected.fe local_doflocal_dof (g)local_dof (g, l)    Returns the number of the node corresponding to the global DOF, g.  If l    is specified the it will contain the local DOF on return.  (The number    of the node is returned rather than the node object itself since the    nodes may have been renumbered.)fe remove_constrainedremove_constrained (K)    Removes the rows and columns of K at all DOFs with a fixed boundary    condition and returns the new matrix.  K is not modified.  K should with    be either a symmetric matrix or a column vector.  The size of K must be    consistent with the definition of the problem.fe renumber_nodesrenumber_nodes ( )    Renumbers the nodes of the current problem using the    Gibbs-Poole-Stockmeyer and Gibbs-King node renumbering algorithms for    bandwidth and profile reduction.  The result is a permutation vector of    the node numbers.fe restore_numbersrestore_numbers (p)    Restores the original node numbering of the current problem.  The    permutation vector is specified by p.  The return value is always null.fe set_upset_up (e)set_up (e, s)    Not available yet.fe solve_displacementssolve_displacements (K, f)    Solves the linear system Kd = f for the vector of global nodal    displacements.  The sizes of the inputs must be consistent with the    definition of the problem.  Additionally, K and f should both be    condensed.  K is expected to be compact.fe zero_constrainedzero_constrained (K)    Zeroes the rows and columns of K at all DOFs with a fixed boundary    condition and returns the new matrix.  K is not modified.  K should with    be either a symmetric matrix or a column vector.  If K is a matrix then    a one is placed on the corresponding diagonal.  The size of K must be    consistent with the definition of the problem.

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