Added off-axis propagation, SPIE scripts

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yosata committed 2020-11-02 17:16:33 +01:00
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import numpy as np
import os
import sys
import matplotlib.pyplot as plt
import matplotlib.cm as cm
sys.path.insert(0, '/Users/joost/Dropbox/Werk/PhD/Analyses/Python/Analytical/Fourier Optics')
from fourierOptics import *
'''
Author: Joost van den Born, PhD student at University of Groningen
Contact: born@astro.rug.nl
Description: Script to plot the results of the centroid shift analysis.
Script made for the SPIE manuscript.
'''
def plot_colourline(x,y,c, ax):
'''
Source: https://stackoverflow.com/questions/36505587/color-line-by-third-variable-python
Function to colour a line according to a thrid variable.
In our case, this will be the Strehl ratio
'''
c = cm.plasma_r(c)
for i in np.arange(len(x)-1):
ax.plot([x[i],x[i+1]], [y[i],y[i+1]], c=c[i])
return
if __name__ == '__main__':
plt.rc('font', family='serif')
plt.rc('text', usetex=True)
# Load in the results from centroid_shift_analysis.py
rms_zern_nm, r_airy_zern_mas, r_err_zern_airy_mas, strehl_list_zern = load_variable('./data/centroid_shift_zernikes.pkl')
rms_psd_nm, r_airy_psd_mas, r_err_psd_airy_mas, strehl_list_psd = load_variable('./data/centroid_shift_psd.pkl')
# Convert the errors to logarithmic space, assuming small errors.
log_err_zern_airy_mas = 0.434 * r_err_zern_airy_mas / r_airy_zern_mas
log_err_psd_airy_mas = 0.434 * r_err_psd_airy_mas / r_airy_psd_mas
# Plot the resulting WFE scaling relation
fig = plt.figure(figsize=(9,7))
ax1 = fig.add_subplot(111)
ax1.errorbar((0.8138)*rms_zern_nm, r_airy_zern_mas, yerr=log_err_zern_airy_mas, color='k',
linestyle='none', capsize=3,
markeredgewidth=1)
ax1.errorbar((0.8138)*rms_psd_nm, r_airy_psd_mas, yerr=log_err_psd_airy_mas, color='k',
linestyle='none', capsize=3,
markeredgewidth=1)
ax1.scatter((0.8138)*rms_zern_nm, r_airy_zern_mas, c=strehl_list_zern, marker='v', label='Zernikes', cmap='plasma_r')
im = ax1.scatter((0.8138)*rms_psd_nm, r_airy_psd_mas, c=strehl_list_psd, marker='o', label='PSD', cmap='plasma_r')
# We colour the lines by their Strehl ratio
plot_colourline((0.8138)*rms_zern_nm, r_airy_zern_mas, strehl_list_zern, ax=ax1)
plot_colourline((0.8138)*rms_psd_nm, r_airy_psd_mas, strehl_list_psd, ax=ax1)
ax1.set_xscale('log')
ax1.set_yscale('log')
ax1.set_xlabel('$\\sigma_{\\mathrm{WFE}}$ (nm)', fontsize=18)
ax1.set_ylabel('Centroid shift (mas)', fontsize=18)
ax1.set_xlim([np.min(rms_zern_nm)*(0.8138), np.max(rms_zern_nm)*(0.8138)])
ax1.legend(fontsize=18)
ax1.grid(True, alpha=0.3, which='major')
ax1.grid(True, alpha=0.1, which='minor')
ax1.tick_params(labelsize=18)
cb = fig.colorbar(im, ax=ax1)
cb.set_label(label='Strehl', size=18)
cb.ax.tick_params(labelsize=18)
plt.savefig('./figures/WFE_scaling_relation_obscured_airy.png', bbox_inches='tight', transparent=True)
plt.savefig('./figures/WFE_scaling_relation_obscured_airy.pdf', bbox_inches='tight', transparent=True)
plt.tight_layout()
plt.show()