#encoding=utf8

import matplotlib
from matplotlib import rc
from matplotlib import pyplot as plt
import numpy as np

rc('lines', linewidth=0.5)
rc('font', family='sans-serif', size=10)
rc('axes', labelsize=10)
rc('xtick', labelsize=9)
rc('ytick', labelsize=9)

golden_mean = (np.sqrt(5)-1.0)/2.0
inches_per_cm = 1.0/2.54
fig_width = 8 * inches_per_cm
fig_height = golden_mean * fig_width
fig = plt.figure(figsize = [fig_width, fig_height])

from colorpy import ciexyz, colormodels

Fs = 2.16e-5 * np.pi;   # Geometrical factor of sun as viewed from Earth
h = 6.63e-34;           # Boltzmann const. [Js]
c = 3.e8;               # speed of light [m/s]
q = 1.602e-19;          # electron charge [C]

def blackbody(wvlgth, temp):
    # per nanometer 1e-9:
    fac = (2 * Fs * h * c**2) / ((wvlgth * 1.e-9)**5)
    return fac / (np.exp(1240./(wvlgth*8.62e-5*temp)) - 1) * 1.e-9

def draw_vis_spec(ax, ymax):
    spectrum = ciexyz.empty_spectrum()[:,0]
    (num_wl,) = spectrum.shape
    rgb_colors = np.empty((num_wl, 3))
    for i in xrange (0, num_wl):
        xyz = ciexyz.xyz_from_wavelength(spectrum[i])
        rgb = colormodels.rgb_from_xyz(xyz)
        rgb_colors [i] = rgb
    rgb_colors /= np.max(rgb_colors) # scale to make brightest rgb value = 1.0
    
    num_points = len(spectrum)
    for i in xrange (0, num_points-1):
        x0 = spectrum[i]
        x1 = spectrum[i+1]
        y0 = 0.0
        y1 = ymax
        poly_x = [x0, x1, x1, x0]
        poly_y = [y0, y0, y1, y1]
        color_string = colormodels.irgb_string_from_rgb(rgb_colors [i])
        ax.fill(poly_x, poly_y, color_string, edgecolor=color_string)

ax = fig.add_subplot(111)

frame = ax.get_frame()
frame.set_facecolor('black')
xmax = 2000
ymax = 2.5

# Visible spectrum:

draw_vis_spec(ax, ymax)

# Blackbody:

temp = 5777
x = np.arange(100, 2000)
y = blackbody(x, temp)
y[-1] = 0.
ax.fill(x, y, '0.5', alpha = 0.7, linewidth = 0.9, edgecolor='yellow', label = 'Svart legeme\n%d K' % temp)

# AM0 spectrum:

d = np.loadtxt('smarts295.ext.txt', skiprows = 1)
x = d[:,0]
y = d[:,1]
y[0] = 0.
y[-1] = 0.
ax.plot(x, y, color='white', linewidth=0.5, label = 'AM0')
ax.set_xlim(0, xmax)
ax.set_xticks(np.arange(0, 1999, 300))
ax.set_ylim(0, ymax)

# Tweak, tweak and annotate:

texty = 2.25
ax.annotate('UV', xy = (50,texty), xytext = (230,texty), xycoords = 'data', 
        horizontalalignment='left', verticalalignment='center', color='#33bb33',
        arrowprops = dict(arrowstyle='->', color='#33bb33'))
#ax.annotate('Synlig', xy=(400,texty), xycoords='data', 
#        horizontalalignment='left', verticalalignment='center', color='white')
ax.annotate(u'Infrarødt', xytext = (720,texty), xy = (1900,texty), xycoords = 'data', 
        horizontalalignment='left', verticalalignment='center', color='#33bb33', 
        arrowprops = dict(arrowstyle='->',color='#33bb33'))

leg = ax.legend(loc='upper right', frameon=False, bbox_to_anchor = (1.0, 0.90) )
txts = leg.get_texts()
for txt in txts:
    txt.set_color('white')
    txt.set_fontsize(9)

ax.tick_params(color='white', labelcolor='black')
for spine in ax.spines.values():
    spine.set_edgecolor('white')
    spine.set_linewidth(1.4)

fig.subplots_adjust(left=0.16, bottom = 0.19, right=0.98, top=0.96)

ax.set_xlabel(u'Bølgelengde [nm]')
ax.set_ylabel(u'Irradians [W/m$^2$/nm]')
fig.savefig('Solar AM0 spectrum with visible spectrum background (no).png',dpi=600)