https://github.com/chill90/BoloCalc
Tip revision: fd51b24110488cea7835ad1b10fb6390066f4586 authored by Charles Hill on 31 March 2020, 06:37:22 UTC
Fixed varying of 'NA' parameter
Fixed varying of 'NA' parameter
Tip revision: fd51b24
sensitivity.py
# Built-in modules
import numpy as np
import functools as ft
import copy as cp
class Sensitivity:
"""
Sensitivity object takes a simulation object, which has information about
the experiment, and calculates the sensitivity
Args:
sim (src.Simulation): parent Simulation object
Attributes:
exp_dir (str): input experiment directory
senses (list): array of output sensitivities
opt_pos (list): array of output optical power arrays
Parents:
sim (src.Simulation): parent Simulation object
exp (src.Experiment): parent Experiment object
"""
def __init__(self, sim):
# Store passed parameters
self.exp = sim.exp
self._log = sim.log
self._phys = sim.phys
self._noise = sim.noise
self._corr = sim.param("corr")
self._nobs = sim.param("nobs")
self._ndet = sim.param("ndet")
# ***** Public methods *****
def sensitivity(self, exp=None):
"""
Calculate sensitivity for a given experiment
Args:
exp (src.Experiment): Experiment to evaluate. Defaults to None,
which triggers evaluating the parent Experiment object
"""
if exp is None:
exp = self.exp
return [[[self.ch_sensitivity(ch) for ch in cam.chs.values()]
for cam in tp.cams.values()]
for tp in exp.tels.values()]
def opt_pow(self):
""" Calculate optical power tables for parent Experiment object """
return [[[self._opt_pow(ch) for ch in cm.chs.values()]
for cm in tp.cams.values()]
for tp in self.exp.tels.values()]
def ch_sensitivity(self, ch):
"""
Calculate channel sensitivity of a specific Channel object
Args:
ch (src.Channel): Channel object
"""
# Calculate optical power
self._calc_popt(ch)
self._calc_rj_temp(ch)
# Calculate NEP
self._calc_photon_NEP(ch)
self._calc_bolo_NEP(ch)
self._calc_read_NEP(ch)
self._calc_tot_NEP(ch)
# Calculte NET
self._calc_NET(ch)
self._calc_NET_RJ(ch)
# Calculate array NET
self._calc_NET_arr(ch)
self._calc_NET_arr_RJ(ch)
# Calculate correlation degradation
self._calc_corr_deg(ch)
# Calculate map depth
self._calc_map_depth(ch)
self._calc_map_depth_RJ(ch)
# Return a list of parameter distributions
return [self._tel_eff_arr.flatten().tolist(),
self._popt_arr.flatten().tolist(),
self._tel_rj_temp.flatten().tolist(),
self._sky_rj_temp.flatten().tolist(),
self._NEP_ph_arr.flatten().tolist(),
self._NEP_bolo_arr.flatten().tolist(),
self._NEP_read_arr.flatten().tolist(),
self._NEP.flatten().tolist(),
self._NET.flatten().tolist(),
self._NET_RJ.flatten().tolist(),
self._NET_arr.flatten().tolist(),
self._NET_arr_RJ.flatten().tolist(),
self._corr_deg.flatten().tolist(),
self._map_depth.flatten().tolist(),
self._map_depth_RJ.flatten().tolist()]
# *** Helper methods ***
def _opt_pow(self, ch):
""" Calculate optical power table for a specific channel """
# Store passed parameters
self._pow_sky_side = []
self._pow_det_side = []
self._eff_det_side = []
for i in range(len(ch.elem)): # nobs
pow_sky_side_1 = []
pow_det_side_1 = []
eff_det_side_1 = []
for j in range(len(ch.elem[i])): # ndet
det_band = np.array(ch.det_arr.dets[j].band)
bw = ch.det_arr.dets[j].param("bw")
pows = []
pow_sky_side_2 = []
pow_det_side_2 = []
eff_sky_side_2 = []
eff_det_side_2 = []
# Store efficiency towards sky and towards detector
for k in range(len(ch.elem[i][j])): # nelem
# Buffer the efficiency array
eff_arr = np.vstack([ch.tran[i][j],
np.array([1. for f in ch.freqs])])
# Efficiency towards the detector
cum_eff_det = ft.reduce(lambda x, y: x*y, eff_arr[k+1:])
eff_det_side_2.append(np.array(cum_eff_det))
# Efficiency towards the sky
if k == 0:
# Zero elements sky side
cum_eff_sky = [[0. for f in ch.freqs]]
elif k == 1:
# One element sky side
cum_eff_sky = [[1. for f in ch.freqs],
[0. for f in ch.freqs]]
else:
cum_eff_sky = [ft.reduce(
lambda x, y: x*y, eff_arr[m+1:k])
if m < k-2 else eff_arr[m+1]
for m in range(k-1)] + [[1. for f in ch.freqs],
[0. for f in ch.freqs]]
eff_sky_side_2.append(cum_eff_sky)
pow = self._phys.bb_pow_spec(
ch.freqs, ch.temp[i][j][k], ch.emis[i][j][k])
pows.append(pow)
# Store band-averaged power from sky and power on detector
# and band-average the efficiencies
for k in range(len(ch.elem[i][j])):
pow_out = np.trapz(pows[k] * eff_det_side_2[k], ch.freqs)
pow_det_side_2.append(pow_out)
eff_det_side_2[k] = (
np.trapz(eff_det_side_2[k], ch.freqs) / bw)
pow_in = sum([np.trapz(
pows[m] * eff_sky_side_2[k][m] *
det_band, ch.freqs)
for m in range(k+1)])
pow_sky_side_2.append(pow_in)
# Force the final efficiency to be 100%
eff_det_side_2[-1] = 1.
pow_sky_side_1.append(pow_sky_side_2)
pow_det_side_1.append(pow_det_side_2)
eff_det_side_1.append(eff_det_side_2)
self._pow_sky_side.append(pow_sky_side_1)
self._pow_det_side.append(pow_det_side_1)
self._eff_det_side.append(eff_det_side_1)
# Build table of optical powers and efficiencies for each element
return self._opt_table()
def _calc_popt(self, ch):
""" Calculate optical power for a specific channel """
self._popt_arr = np.array([[self._popt(
ch.elem[i][j], ch.emis[i][j], ch.tran[i][j],
ch.temp[i][j], ch.freqs)
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_rj_temp(self, ch):
""" Calculate telescope RJ temp for a specific temperature """
n_sky_elem = self._num_sky_elem(ch)
# Telescope efficiency
self._tel_eff_arr = np.array([[self._eff(
ch.tran[i][j][n_sky_elem-1:],
ch.freqs, ch.det_arr.dets[j].param("bw"))
for j in range(self._ndet)]
for i in range(self._nobs)])
# Telescope temperature
self._tel_rj_temp = np.array([[self._rj_temp(
ch.elem[i][j][n_sky_elem:],
ch.emis[i][j][n_sky_elem:],
ch.tran[i][j][n_sky_elem:],
ch.temp[i][j][n_sky_elem:],
ch.freqs, self._tel_eff_arr[i][j],
ch.det_arr.dets[j].param("bw"))
for j in range(self._ndet)]
for i in range(self._nobs)])
# Sky temperature
self._sky_rj_temp = np.array([[self._rj_temp(
ch.elem[i][j][:n_sky_elem],
ch.emis[i][j][:n_sky_elem],
ch.tran[i][j],
ch.temp[i][j][:n_sky_elem],
ch.freqs, self._tel_eff_arr[i][j],
ch.det_arr.dets[j].param("bw"))
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_photon_NEP(self, ch):
""" Calculate photon NEP for a specific channel """
if self._corr:
pass_ch = ch
else:
pass_ch = None
NEP_ph_out = np.array([[self._photon_NEP(
ch.elem[i][j], ch.emis[i][j], ch.tran[i][j],
ch.temp[i][j], ch.freqs, pass_ch)
for j in range(self._ndet)]
for i in range(self._nobs)])
# pylint: disable=unbalanced-tuple-unpacking
NEP_ph_arr, NEP_ph_arr_corr = np.split(NEP_ph_out, 2, axis=2)
self._NEP_ph_arr = np.reshape(
NEP_ph_arr, np.shape(NEP_ph_arr)[:2])
self._NEP_ph_arr_corr = np.reshape(
NEP_ph_arr_corr, np.shape(NEP_ph_arr_corr)[:2])
return
def _calc_bolo_NEP(self, ch):
""" Calculate bolometer NEP for a specific channel """
self._NEP_bolo_arr = np.array([[self._bolo_NEP(
self._popt_arr[i][j], ch.det_arr.dets[j])
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_read_NEP(self, ch):
""" Calculate readout NEP for a specific channel """
NEP_read_arr = np.array([[self._read_NEP(
self._popt_arr[i][j], ch.det_arr.dets[j])
for j in range(self._ndet)]
for i in range(self._nobs)])
if np.any(np.isin(NEP_read_arr.astype(str), ['NA'])):
self._NEP_read_arr = np.array([[np.sqrt(
(1. + ch.det_arr.dets[j].param("read_frac"))**2 - 1.) *
np.sqrt(self._NEP_ph_arr[i][j]**2 +
self._NEP_bolo_arr[i][j]**2)
for j in range(self._ndet)]
for i in range(self._nobs)])
else:
self._NEP_read_arr = NEP_read_arr
return
def _calc_tot_NEP(self, ch):
""" Calculate total NEP for a specific channel """
self._NEP = np.sqrt(self._NEP_ph_arr**2 +
self._NEP_bolo_arr**2 +
self._NEP_read_arr**2)
# Total NEP with correlation adjustment
self._NEP_corr = np.sqrt(self._NEP_ph_arr_corr**2 +
self._NEP_bolo_arr**2 +
self._NEP_read_arr**2)
return
def _calc_NET(self, ch):
""" Calculate NET for a specific channel """
# Total NET
self._NET = np.array([[self._noise.NET_from_NEP(
self._NEP[i][j], ch.freqs, np.prod(ch.tran[i][j], axis=0),
ch.cam.param("opt_coup"))
for j in range(self._ndet)]
for i in range(self._nobs)]) * (
ch.cam.tel.param("net_mgn"))
# Total NET with correlation adjustment
self._NET_corr = np.array([[self._noise.NET_from_NEP(
self._NEP_corr[i][j], ch.freqs, np.prod(ch.tran[i][j], axis=0),
ch.cam.param("opt_coup"))
for j in range(self._ndet)]
for i in range(self._nobs)]) * (
ch.cam.tel.param("net_mgn"))
return
def _calc_NET_RJ(self, ch):
""" Calculate RJ NET for a specific channel """
self._NET_RJ = np.array([[self._Trj_over_Tcmb(
ch.freqs)*self._NET[i][j]
for j in range(self._ndet)]
for i in range(self._nobs)])
self._NET_corr_RJ = np.array([[self._Trj_over_Tcmb(
ch.freqs)*self._NET_corr[i][j]
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_NET_arr(self, ch):
""" Calcualte array NET for a specific channel """
self._NET_arr = np.array([[self._noise.NET_arr(
self._NET_corr[i][j], ch.param("ndet"), ch.param("yield"))
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_NET_arr_RJ(self, ch):
""" Calculate array NET RJ for a specific channel """
self._NET_arr_RJ = np.array([[self._noise.NET_arr(
self._NET_corr_RJ[i][j], ch.param("ndet"), ch.param("yield"))
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_corr_deg(self, ch):
""" Calculate correlation factor for a specific channel """
self._corr_deg = np.array([[self._NET_corr[i][j] / self._NET[i][j]
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_map_depth(self, ch):
""" Calculate map depth for a specific channel """
tel = ch.cam.tel
self._map_depth = np.array([[self._noise.map_depth(
self._NET_arr[i][j], tel.param("fsky"),
tel.param("tobs"), tel.param("obs_eff"))
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _calc_map_depth_RJ(self, ch):
""" Calculate RJ map depth for a specific channel """
tel = ch.cam.tel
self._map_depth_RJ = np.array([[self._noise.map_depth(
self._NET_arr_RJ[i][j], tel.param("fsky"),
tel.param("tobs"), tel.param("obs_eff"))
for j in range(self._ndet)]
for i in range(self._nobs)])
return
def _eff(self, tran, freqs, bw):
""" Calculate cumulative efficiency """
tot_eff = np.trapz(np.prod(tran, axis=0), freqs) / bw
return tot_eff
def _popt(self, elem, emis, tran, temp, freqs):
""" Calculate optical power """
buf_tran = self._buffer_tran(tran, freqs)
tot_pow = np.sum([np.trapz(
self._phys.bb_pow_spec(
freqs, temp[i], emis[i] *
np.prod(buf_tran[i+1:], axis=0)), freqs)
for i in range(len(elem))])
return tot_pow
def _rj_temp(self, elem, emis, tran, temp, freqs, eff, bw):
""" Calculate RJ temperature """
opt_pow = self._popt(elem, emis, tran, temp, freqs)
rj_temp = self._phys.rj_temp(opt_pow, bw, eff)
return rj_temp
def _photon_NEP(self, elem, emis, tran, temp, freqs, ch=None):
""" Calculate photon NEP """
tran = self._buffer_tran(tran, freqs)
if ch:
corrs = True
else:
corrs = False
pow_ints = np.array([self._phys.bb_pow_spec(
freqs, temp[i], emis[i]*np.prod(tran[i+1:], axis=0))
for i in range(len(elem))])
if corrs:
# Photon NEP both without and with correlations
NEP_ph, NEP_ph_arr = self._noise.photon_NEP(
pow_ints, freqs, elem, (
ch.param("pix_sz") /
float(ch.cam.param("fnum") * self._phys.lamb(
ch.param("bc")))))
else:
# Both outputs are identical
NEP_ph, NEP_ph_arr = self._noise.photon_NEP(pow_ints, freqs)
return NEP_ph, NEP_ph_arr
def _bolo_NEP(self, opt_pow, det):
""" Calculate bolometer NEP """
if 'NA' in str(det.param("g")):
if 'NA' in str(det.param("psat")):
g = self._noise.G(
det.param("psat_fact") * opt_pow, det.param("n"),
det.param("tb"), det.param("tc"))
else:
g = self._noise.G(
det.param("psat"), det.param("n"),
det.param("tb"), det.param("tc"))
else:
g = det.param("g")
if 'NA' in str(det.param("flink")):
return self._noise.bolo_NEP(
self._noise.Flink(
det.param("n"), det.param("tb"), det.param("tc")),
g, det.param("tc"))
else:
return self._noise.bolo_NEP(
det.param("flink"), g, det.param("tc"))
def _read_NEP(self, opt_pow, det):
""" Calculate readout NEP """
if 'NA' in str(det.param("nei")):
return 'NA'
elif 'NA' in str(det.param("bolo_r")):
return 'NA'
elif 'NA' in str(det.param("psat")):
p_bias = (det.param("psat_fact") - 1.) * opt_pow
else:
if opt_pow >= det.param("psat"):
return 0.
else:
p_bias = det.param("psat") - opt_pow
if 'NA' in str(det.param("sfact")):
sfact = 1.
else:
sfact = det.param("sfact")
return self._noise.read_NEP(
p_bias, det.param("bolo_r"),
det.param("nei"), sfact)
def _Trj_over_Tcmb(self, freqs):
""" Convert to RJ temperature from CMB temperature """
factor_spec = self._phys.Trj_over_Tb(freqs, self._phys.Tcmb)
bw = freqs[-1] - freqs[0]
factor = np.trapz(factor_spec, freqs)/bw
return factor
def _buffer_tran(self, tran, freqs):
""" Function to buffer the transmission array with ones """
out_tran = cp.copy(np.insert(
tran, len(tran), [1. for f in freqs], axis=0))
return np.array(out_tran).astype(np.float)
def _opt_table(self):
""" Calculate optial power table """
shape = np.shape(self._pow_sky_side)
new_shape = (shape[0] * shape[1], shape[2])
pow_sky_side = np.transpose(np.reshape(self._pow_sky_side, new_shape))
pow_det_side = np.transpose(np.reshape(self._pow_det_side, new_shape))
eff_det_side = np.transpose(np.reshape(self._eff_det_side, new_shape))
return [pow_sky_side,
pow_det_side,
eff_det_side]
def _num_sky_elem(self, ch):
""" Discern the number of sky optical elements """
site = ch.cam.tel.param("site").upper()
infg = ch.cam.tel.exp.sim.param("infg")
if site == "ROOM":
nelem = 1
elif site == "SPACE":
if infg:
nelem = 3
else:
nelem = 1
else:
if infg:
nelem = 4
else:
nelem = 2
return nelem