tinypythonpanadapter/iq_dsp.py

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4.1 KiB
Python
Executable File

#!/usr/bin/env python
# Program iq_dsp.py - Compute spectrum from I/Q data.
# Copyright (C) 2013-2014 Martin Ewing
#
# 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/>.
#
# Contact the author by e-mail: aa6e@arrl.net
#
# Part of the iq.py program.
# HISTORY
# 01-04-2014 Initial Release
import math, time
import numpy as np
import numpy.fft as fft
class DSP(object):
def __init__(self, opt):
self.opt = opt
self.stats = list()
# This is dB output for full scale 16bit input = max signal.
self.db_adjust = 20. * math.log10(self.opt.size * 2**15)
self.rejected_count = 0
self.led_clip_ct = 0
# Use "Hanning" window function
self.w = np.empty(self.opt.size)
for i in range(self.opt.size):
self.w[i] = 0.5 * (1. - math.cos((2*math.pi*i)/(self.opt.size-1)))
return
def GetLogPowerSpectrum(self, data):
size = self.opt.size # size of FFT in I,Q samples.
power_spectrum = np.zeros(size)
# Time-domain analysis: Often we have long normal signals interrupted
# by huge wide-band pulses that degrade our power spectrum average.
# We find the "normal" signal level, by computing the median of the
# absolute value. We only do this for the first buffer of a chunk,
# using the median for the remaining buffers in the chunk.
# A "noise pulse" is a signal level greater than some threshold
# times the median. When such a pulse is found, we skip the current
# buffer. It would be better to blank out just the pulse, but that
# would be more costly in CPU time.
# Find the median abs value of first buffer to use for this chunk.
td_median = np.median(np.abs(data[:size]))
# Calculate our current threshold relative to measured median.
td_threshold = self.opt.pulse * td_median
nbuf_taken = 0 # Actual number of buffers accumulated
for ic in range(self.opt.buffers):
td_segment = data[ic*size:(ic+1)*size]
td_max = np.amax(np.abs(td_segment)) # Do we have a noise pulse?
if td_max < td_threshold: # No, get pwr spectrum etc.
# EXPERIMENTAL TAPER
td_segment *= self.w
fd_spectrum = fft.fft(td_segment)
# Frequency-domain:
# Rotate array to place 0 freq. in center. (It was at left.)
fd_spectrum_rot = np.fft.fftshift(fd_spectrum)
# Compute the real-valued squared magnitude (ie power) and
# accumulate into pwr_acc.
# fastest way to sum |z|**2 ??
nbuf_taken += 1
power_spectrum = power_spectrum + \
np.real(fd_spectrum_rot*fd_spectrum_rot.conj())
else: # Yes, abort buffer.
self.rejected_count += 1
self.led_clip_ct = 1 # flash a red light
#if DEBUG: print "REJECT! %d" % self.rejected_count
if nbuf_taken > 0:
power_spectrum = power_spectrum / nbuf_taken # normalize the sum.
else:
power_spectrum = np.ones(size) # if no good buffers!
# Convert to dB. Note log(0) = "-inf" in Numpy. It can happen if ADC
# isn't working right. Numpy issues a warning.
log_power_spectrum = 10. * np.log10(power_spectrum)
return log_power_spectrum - self.db_adjust # max poss. signal = 0 dB