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-rwxr-xr-xgr-radio-astronomy/src/python/usrp_psr_receiver.py34
1 files changed, 6 insertions, 28 deletions
diff --git a/gr-radio-astronomy/src/python/usrp_psr_receiver.py b/gr-radio-astronomy/src/python/usrp_psr_receiver.py
index 759022cfb..3c7dedac8 100755
--- a/gr-radio-astronomy/src/python/usrp_psr_receiver.py
+++ b/gr-radio-astronomy/src/python/usrp_psr_receiver.py
@@ -356,17 +356,8 @@ class app_flow_graph(stdgui.gui_flow_graph):
self.second = gr.fir_filter_fff (int(p), second_filter)
self.third = gr.fir_filter_fff (10, third_filter)
- # Split complex USRP stream into a pair of floats
- self.splitter = gr.complex_to_float (1);
-
- # I squarer (detector)
- self.multI = gr.multiply_ff();
-
- # Q squarer (detector)
- self.multQ = gr.multiply_ff();
-
- # Adding squared I and Q to produce instantaneous signal power
- self.adder = gr.add_ff();
+ # Detector
+ self.detector = gr.complex_to_mag_squared()
self.enable_comb_filter = False
# Epoch folder comb filter
@@ -402,25 +393,12 @@ class app_flow_graph(stdgui.gui_flow_graph):
# Start connecting configured modules in the receive chain
#
- # Connect raw USRP to de-dispersion filter, complex->float splitter
- self.connect(self.u, self.dispfilt, self.splitter)
-
- # Connect splitter outputs to multipliers
- # First do I^2
- self.connect((self.splitter, 0), (self.multI,0))
- self.connect((self.splitter, 0), (self.multI,1))
-
- # Then do Q^2
- self.connect((self.splitter, 1), (self.multQ,0))
- self.connect((self.splitter, 1), (self.multQ,1))
-
- # Then sum the squares
- self.connect(self.multI, (self.adder,0))
- self.connect(self.multQ, (self.adder,1))
+ # Connect raw USRP to de-dispersion filter, detector
+ self.connect(self.u, self.dispfilt, self.detector)
- # Connect detector/adder output to FIR LPF
+ # Connect detector output to FIR LPF
# in two stages, followed by the FFT scope
- self.connect(self.adder, self.first,
+ self.connect(self.detector, self.first,
self.second, self.third, self.scope)
# Connect audio output