Source code for compass.ocean.tests.global_convergence.cosine_bell.analysis

import warnings

import matplotlib.pyplot as plt
import numpy as np
import xarray as xr

from compass.step import Step


[docs] class Analysis(Step): """ A step for visualizing the output from the cosine bell test case Attributes ---------- resolutions : list of int The resolutions of the meshes that have been run icosahedral : bool Whether to use icosahedral, as opposed to less regular, JIGSAW meshes """
[docs] def __init__(self, test_case, resolutions, icosahedral): """ Create the step Parameters ---------- test_case : compass.ocean.tests.global_convergence.cosine_bell.CosineBell The test case this step belongs to resolutions : list of int The resolutions of the meshes that have been run icosahedral : bool Whether to use icosahedral, as opposed to less regular, JIGSAW meshes """ # noqa: E501 super().__init__(test_case=test_case, name='analysis') self.resolutions = resolutions self.icosahedral = icosahedral for resolution in resolutions: if icosahedral: mesh_name = f'Icos{resolution}' else: mesh_name = f'QU{resolution}' self.add_input_file( filename=f'{mesh_name}_init.nc', target=f'../{mesh_name}/init/initial_state.nc') self.add_input_file( filename=f'{mesh_name}_output.nc', target=f'../{mesh_name}/forward/output.nc') self.add_output_file('convergence.png')
[docs] def run(self): """ Run this step of the test case """ plt.switch_backend('Agg') resolutions = self.resolutions xdata = list() ydata = list() for res in resolutions: if self.icosahedral: mesh_name = f'Icos{res}' else: mesh_name = f'QU{res}' rmseValue, nCells = self.rmse(mesh_name) xdata.append(nCells) ydata.append(rmseValue) xdata = np.asarray(xdata) ydata = np.asarray(ydata) p = np.polyfit(np.log10(xdata), np.log10(ydata), 1) conv = abs(p[0]) * 2.0 yfit = xdata ** p[0] * 10 ** p[1] plt.loglog(xdata, yfit, 'k') plt.loglog(xdata, ydata, 'or') plt.annotate('Order of Convergence = {}'.format(np.round(conv, 3)), xycoords='axes fraction', xy=(0.3, 0.95), fontsize=14) plt.xlabel('Number of Grid Cells', fontsize=14) plt.ylabel('L2 Norm', fontsize=14) plt.savefig('convergence.png', bbox_inches='tight', pad_inches=0.1) section = self.config['cosine_bell'] if self.icosahedral: conv_thresh = section.getfloat('icos_conv_thresh') conv_max = section.getfloat('icos_conv_max') else: conv_thresh = section.getfloat('qu_conv_thresh') conv_max = section.getfloat('qu_conv_max') if conv < conv_thresh: raise ValueError(f'order of convergence ' f' {conv} < min tolerence {conv_thresh}') if conv > conv_max: warnings.warn(f'order of convergence ' f'{conv} > max tolerence {conv_max}')
[docs] def rmse(self, mesh_name): """ Compute the RMSE for a given resolution Parameters ---------- mesh_name : str The name of the mesh Returns ------- rmseValue : float The root-mean-squared error nCells : int The number of cells in the mesh """ config = self.config latCent = config.getfloat('cosine_bell', 'lat_center') lonCent = config.getfloat('cosine_bell', 'lon_center') radius = config.getfloat('cosine_bell', 'radius') psi0 = config.getfloat('cosine_bell', 'psi0') pd = config.getfloat('cosine_bell', 'vel_pd') init = xr.open_dataset(f'{mesh_name}_init.nc') # find time since the beginning of run ds = xr.open_dataset(f'{mesh_name}_output.nc') for j in range(len(ds.xtime)): tt = str(ds.xtime[j].values) tt.rfind('_') DY = float(tt[10:12]) - 1 if DY == pd: sliceTime = j break HR = float(tt[13:15]) MN = float(tt[16:18]) t = 86400.0 * DY + HR * 3600. + MN # find new location of blob center # center is based on equatorial velocity R = init.sphere_radius distTrav = 2.0 * 3.14159265 * R / (86400.0 * pd) * t # distance in radians is distRad = distTrav / R newLon = lonCent + distRad if newLon > 2.0 * np.pi: newLon -= 2.0 * np.pi # construct analytic tracer tracer = np.zeros_like(init.tracer1[0, :, 0].values) latC = init.latCell.values lonC = init.lonCell.values temp = R * np.arccos(np.sin(latCent) * np.sin(latC) + np.cos(latCent) * np.cos(latC) * np.cos( lonC - newLon)) mask = temp < radius tracer[mask] = psi0 / 2.0 * ( 1.0 + np.cos(3.1415926 * temp[mask] / radius)) # oad forward mode data tracerF = ds.tracer1[sliceTime, :, 0].values rmseValue = np.sqrt(np.mean((tracerF - tracer)**2)) init.close() ds.close() return rmseValue, init.dims['nCells']