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| author | mleech | 2006-10-04 14:36:13 +0000 |
|---|---|---|
| committer | mleech | 2006-10-04 14:36:13 +0000 |
| commit | c7be5804b32bcf19739297b04f3d811bee1a47fb (patch) | |
| tree | 2d1d5f6f91a19e45534095cb26e3daea30d49e45 /gr-radio-astronomy/src/python/usrp_psr_receiver.py | |
| parent | 58d96ee6c7c8992eaf9659668cc70530ef2f3171 (diff) | |
| download | gnuradio-c7be5804b32bcf19739297b04f3d811bee1a47fb.tar.gz gnuradio-c7be5804b32bcf19739297b04f3d811bee1a47fb.tar.bz2 gnuradio-c7be5804b32bcf19739297b04f3d811bee1a47fb.zip | |
Changed data logging significantly, in that for continuum data, the data
logging is more directly plugged into the signal-processing chain,
rather than being a side-effect of plotting. For spectral data, had it
copy spectral bins into a data buffer that gets dumped once per second
in the UI, same as continuum data.
Added --calib_coeff and --calib_offset command-line parameters to scale
the output of the continuum detector.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3706 221aa14e-8319-0410-a670-987f0aec2ac5
Diffstat (limited to 'gr-radio-astronomy/src/python/usrp_psr_receiver.py')
| -rwxr-xr-x | gr-radio-astronomy/src/python/usrp_psr_receiver.py | 4 |
1 files changed, 2 insertions, 2 deletions
diff --git a/gr-radio-astronomy/src/python/usrp_psr_receiver.py b/gr-radio-astronomy/src/python/usrp_psr_receiver.py index cd2a182d1..91cb2e7ef 100755 --- a/gr-radio-astronomy/src/python/usrp_psr_receiver.py +++ b/gr-radio-astronomy/src/python/usrp_psr_receiver.py @@ -95,7 +95,7 @@ class app_flow_graph(stdgui.gui_flow_graph): self.reflevel = options.reflevel self.divbase = options.divbase self.division = options.division - self.audiodev = options.audio_dev + self.audiodev = options.audio_source # Low-pass cutoff for post-detector filter # Set to 100Hz usually, since lots of pulsars fit in this @@ -295,7 +295,7 @@ class app_flow_graph(stdgui.gui_flow_graph): self.scope = ra_fftsink.ra_fft_sink_f (self, panel, fft_size=int(options.fft_size), sample_rate=PULSAR_MAX_FREQ*2, title="Post-detector spectrum", - cfunc=self.pulsarfunc, xydfunc=self.xydfunc, fft_rate=200) + ofunc=self.pulsarfunc, xydfunc=self.xydfunc, fft_rate=200) # # Tell scope we're looking from DC to PULSAR_MAX_FREQ |