pycsa.core.fourier¶
Classes
|
Fourier transformer class |
- class pycsa.core.fourier.f_trans(nhar_i, nhar_j, ctx=None, buffer_pool=None)¶
Fourier transformer class
- __init__(nhar_i, nhar_j, ctx=None, buffer_pool=None)¶
Initalises a discrete spectral space with the corresponding Fourier coefficients spanning
nhar_iandnhar_j.- Parameters:
nhar_i (int) – number of spectral modes in the first horizontal direction
nhar_j (int) – number of spectral modes in the second horizontal direction
ctx (ComputeContext, optional) – Compute context bundling the buffer pool (and other per-task resources). Default-constructed if absent.
buffer_pool (BufferPool, optional) – Deprecated. Pass
ctx=ComputeContext(buffer_pool=...)instead. Retained as a compatibility alias for one release.
- set_kls(k_rng, l_rng, recompute_nhij=True, components='imag')¶
Method to select a smaller subset of the dense spectral space, e.g., in the Second Approximation step of the algorithm if the First Approximation is computed with a fast-Fourier transform.
- Parameters:
k_rng (list) – list containing the selected k-wavenumber indices
l_rng (list) – list containing the selected l-wavenumber indices
recompute_nhij (bool, optional) – resets
nhar_iandnhar_j, by default Truecomponents (str, optional) – real recomputes the spectral space comprising only real spectral components, by default ‘imag’
- do_full(cell, grad=False)¶
Assembles the sine and cosine terms that make up the Fourier coefficients in the
Mmatrix required in thelinear regressioncomputation:\[M a_m =h\]- Parameters:
cell (
pycsa.data.cell.topo_cellinstance) – cell object instancegrad (bool, optional) – if True, assemble the terms over the cell’s gradient coordinates (
grad_lon/grad_lat) instead of the plain coordinates, selecting the gradient spectral terms; by default False
- do_axial(cell, alpha=0.0)¶
Computes spectral modes along the
(k,l)-axes.Deprecated since version 0.90.0.
- do_cg_spsp(cell)¶
Computes the coarse-grained sparse spectral space
Deprecated since version 0.90.0.
- get_freq_grid(a_m)¶
Assembles a dense representation of the sparse spectral space given the Fourier amplitudes computed in the linear regression step.
- Parameters:
a_m (list) – list of (sparse) Fourier amplitudes
- Returns:
complex 2-D array of shape
(nhar_j, nhar_i)holding the dense Fourier coefficients. The same array is also cached on the instance asself.ampls.- Return type:
np.ndarray