2 ##################################################
3 # Gnuradio Python Flow Graph
5 # Author: Achilleas Anastasopoulos
6 # Description: gnuradio flow graph
7 # Generated: Thu Feb 19 23:16:23 2009
8 ##################################################
10 from gnuradio import gr
11 from gnuradio import trellis
12 from gnuradio.gr import firdes
13 from grc_gnuradio import blks2 as grc_blks2
18 from gnuradio import trellis
20 def run_test(seed,blocksize):
23 ##################################################
25 ##################################################
33 f = trellis.fsm(P,M,L)
36 #p = numpy.ones(Q)/(2.0)
37 #q = numpy.cumsum(p)/(1.0*Q)
41 tt=numpy.arange(0,L*Q)/(1.0*Q)-L/2.0;
43 p=(0.5*scipy.stats.erfc(2*math.pi*BT*(tt-0.5)/math.sqrt(math.log(2.0))/math.sqrt(2.0))-0.5*scipy.stats.erfc(2*math.pi*BT*(tt+0.5)/math.sqrt(math.log(2.0))/math.sqrt(2.0)))/2.0;
50 (f0T,SS,S,F,Sf,Ff,N) = fsm_utils.make_cpm_signals(K,P,M,L,q,frac)
53 Ffa = numpy.insert(Ff,Q,numpy.zeros(N),axis=0)
55 MF = numpy.fliplr(numpy.transpose(Ffa))
57 E = numpy.sum(numpy.abs(Sf)**2,axis=0)
58 Es = numpy.sum(E)/f.O()
61 constellation = numpy.reshape(numpy.transpose(Sf),N*f.O())
65 #print numpy.max(numpy.abs(SS - numpy.dot(Ff , Sf)))
68 N0 = Es * 10.0**(-(1.0*EsN0_db)/10.0)
73 numpy.random.seed(seed*666)
74 data = numpy.random.randint(0, M, head+blocksize+tail+1)
75 #data = numpy.zeros(blocksize+1+head+tail,'int')
78 for i in range(tail+1):
83 ##################################################
85 ##################################################
86 random_source_x_0 = gr.vector_source_b(data, False)
87 gr_chunks_to_symbols_xx_0 = gr.chunks_to_symbols_bf((-1, 1), 1)
88 gr_interp_fir_filter_xxx_0 = gr.interp_fir_filter_fff(Q, p)
89 gr_frequency_modulator_fc_0 = gr.frequency_modulator_fc(2*math.pi*h*(1.0/Q))
91 gr_add_vxx_0 = gr.add_vcc(1)
92 gr_noise_source_x_0 = gr.noise_source_c(gr.GR_GAUSSIAN, (N0/2.0)**0.5, -long(seed))
94 gr_multiply_vxx_0 = gr.multiply_vcc(1)
95 gr_sig_source_x_0 = gr.sig_source_c(Q, gr.GR_COS_WAVE, -f0T, 1, 0)
96 # only works for N=2, do it manually for N>2...
97 gr_fir_filter_xxx_0_0 = gr.fir_filter_ccc(Q, MF[0].conjugate())
98 gr_fir_filter_xxx_0_0_0 = gr.fir_filter_ccc(Q, MF[1].conjugate())
99 gr_streams_to_stream_0 = gr.streams_to_stream(gr.sizeof_gr_complex*1, N)
100 gr_skiphead_0 = gr.skiphead(gr.sizeof_gr_complex*1, N*(1+0))
101 viterbi = trellis.viterbi_combined_cb(f, head+blocksize+tail, 0, -1, N, constellation, trellis.TRELLIS_EUCLIDEAN)
103 gr_vector_sink_x_0 = gr.vector_sink_b()
105 ##################################################
107 ##################################################
108 tb.connect((random_source_x_0, 0), (gr_chunks_to_symbols_xx_0, 0))
109 tb.connect((gr_chunks_to_symbols_xx_0, 0), (gr_interp_fir_filter_xxx_0, 0))
110 tb.connect((gr_interp_fir_filter_xxx_0, 0), (gr_frequency_modulator_fc_0, 0))
111 tb.connect((gr_frequency_modulator_fc_0, 0), (gr_add_vxx_0, 0))
112 tb.connect((gr_noise_source_x_0, 0), (gr_add_vxx_0, 1))
113 tb.connect((gr_add_vxx_0, 0), (gr_multiply_vxx_0, 0))
114 tb.connect((gr_sig_source_x_0, 0), (gr_multiply_vxx_0, 1))
115 tb.connect((gr_multiply_vxx_0, 0), (gr_fir_filter_xxx_0_0, 0))
116 tb.connect((gr_multiply_vxx_0, 0), (gr_fir_filter_xxx_0_0_0, 0))
117 tb.connect((gr_fir_filter_xxx_0_0, 0), (gr_streams_to_stream_0, 0))
118 tb.connect((gr_fir_filter_xxx_0_0_0, 0), (gr_streams_to_stream_0, 1))
119 tb.connect((gr_streams_to_stream_0, 0), (gr_skiphead_0, 0))
120 tb.connect((gr_skiphead_0, 0), (viterbi, 0))
121 tb.connect((viterbi, 0), (gr_vector_sink_x_0, 0))
125 dataest = gr_vector_sink_x_0.data()
127 #print numpy.array(dataest)
130 for i in range(blocksize):
131 if data[head+i] != dataest[head+i]:
138 if __name__ == '__main__':
142 for i in range(10000):
143 (s,e) = run_test(i,blocksize)
147 print i+1,ss,ee,(1.0*ss)/(i+1)/(1.0*blocksize),(1.0*ee)/(i+1)
148 print i+1,ss,ee,(1.0*ss)/(i+1)/(1.0*blocksize),(1.0*ee)/(i+1)