forked from geoxiyang/FluxCourse
-
Notifications
You must be signed in to change notification settings - Fork 0
/
leaf_SIF_tools.py
160 lines (111 loc) · 4.97 KB
/
leaf_SIF_tools.py
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
#
# Copyright 2019 University of Virginia
#
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with this program. If not, see <http://www.gnu.org/licenses/>.
#
# Author: Xi Yang, xiyang@virginia.edu
# the first function is to read a spectrum txt file with standard output,
# and return the digital numbers, wavelengths, and the integration time
import numpy as np
import pandas as pd
import glob
from scipy.optimize import curve_fit
from matplotlib.figure import Figure
from matplotlib.backends.backend_agg import FigureCanvasAgg as FigureCanvas
def read_rawspec(path):
files = glob.glob(path)
spectrum = pd.DataFrame(columns=['wavelength'])
IT = pd.DataFrame(columns=['IT'])
file_i = 0
IT['IT'] = [0.0]
for file in files:
# First read the IT
text_file = open(file,'r')
lines = text_file.readlines()
IT.insert(file_i+1,'IT'+str(file_i),float(lines[6][24:-1]))
# Read the spectrum and wavelength
raw = np.loadtxt(file,delimiter='\t',skiprows =14)
spectrum.insert(file_i+1,'DN'+str(file_i), raw[:,1])
spectrum['wavelength'] = raw[:,0]
file_i = file_i + 1
return spectrum, IT
def SIF_SFM(leaf_radiance,panel_radiance,wavelength):
# For simplicity, we just use a simple version of SIF retrieval based on SFM
o2a_index = (wavelength > 759.00) & (wavelength < 767.76)
plot_index= (wavelength > 730.00) & (wavelength < 780.00)
b755_index= (wavelength > 754.00) & (wavelength < 756.00)
s_bands = wavelength[o2a_index]
p_value = panel_radiance[o2a_index]
xdata = np.zeros((2, len(s_bands)))
xdata[0, :], xdata[1, :] = s_bands, p_value
ydata = leaf_radiance[o2a_index]
x0 = [0.1, 0.1, 0.1, 0.1]
popt, pcov = curve_fit(fit_o2a, xdata, ydata, p0=x0, method='lm',
xtol=1e-10, ftol=1e-10)
wl = 760.0
sif_o2a = popt[2] + wl * popt[3]
# assuming that the panel radiance values have already been multiplied by Pi
refl = leaf_radiance/panel_radiance
irra755 = np.mean(panel_radiance[b755_index])
rad755 = np.mean(leaf_radiance[b755_index])
fig = Figure()
canvas = FigureCanvas(fig)
ax0 = fig.add_subplot(211)
ax0.plot(wavelength[plot_index], refl[plot_index], color='r')
ax0.set_ylabel('reflectance, PI*VEG/SKY')
ax0.set_title("SIF760=%5.2f; Rad755=%.2f"% (sif_o2a, rad755), fontsize=9)
ax0.locator_params(nbins=5, axis='y')
ax1 = fig.add_subplot(212, sharex=ax0)
ax2 = ax1.twinx()
lns1 = ax1.plot(wavelength[plot_index], leaf_radiance[plot_index],
label='leaf', color='m')
lns2 = ax2.plot(wavelength[plot_index], panel_radiance[plot_index],
label='panel', color='k')
ax1.locator_params(nbins=5, axis='y')
ax2.locator_params(nbins=5, axis='y')
ax1.set_xlabel('Wavelength(nm)')
ax1.set_ylabel('leaf, W/m2/nm/sr', color='m')
ax2.set_ylabel('panel, W/m2/nm', color='k')
ax1.tick_params('y', colors='m')
ax2.tick_params('y', colors='k')
lns = lns1 + lns2
labs = [l.get_label() for l in lns]
ax1.legend(lns, labs, loc=0)
frame = ax1.get_legend().get_frame()
frame.set_linewidth(0.5)
# fig.text(0.5, 0.95, dt, horizontalalignment='center', transform=ax0.transAxes)
fig.subplots_adjust()
return (sif_o2a,fig)
def DNtoRad(light,dark,intTime,calib_factor,calib_intTime):
int_conv = np.divide(calib_intTime,intTime)
cal_spec = np.array(calib_factor * int_conv[0])
radiance = (light - dark) * cal_spec
return radiance
def fit_o2a(xdata, a, b, c, d):
''' LL-fit
L(w) = r(w)*E(w)/pi + F(w)
w : wavelength
r : reflectance, don't include the emission component
E : total solar irradiance incident on the target
F : fluorescence
L(w) = r_mod(w)*E(w)/pi + F_mod(w) + error(w)
r_mod : r_mod(w) = a + b*w ; linear
F_mod : F_mod(w) = c + d*w ; linear
L(w) = (a + b*w)*E(w) / pi + c + d*w
'''
# O2A we use linear for Fmod, linear for rmod
L = (a + b * xdata[0, :]) * xdata[1, :] / np.pi + c + xdata[0, :] * d
# incoming radiance measured by reflectance panel
# f = (x(1)+xdata(1,:).*x(2)).*xdata(2,:) + (x(3)+xdata(1,:).*x(4));
return L