Age | Commit message (Collapse) | Author |
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parameter better.
The number of output items is now set based on the d_osps and the check in the work function is not needed (actually, that check was wrong and should never have worked correctly, anyway).
This commit also changes the number of samples needed in the QA code for the constellation receiver for a faster test.
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The intent of this block is to be able to pass messages containing the SNR at a set number of samples.
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arg.
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'snr'). The number of samples between when the tag is sent is set in the constructor (default = 10000) and can be changed.
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complex vectors.
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them. Also set the alpha value to a default of 0.001; most won't need to change this.
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M2M4 type that allows the user to set the kurtosis of the signal and noise, if known, to work with non-MPSK and non-AWGN channels (untested).
Also, the technique is signal to variation ratio (SVR), not SVN. Couldn't read my own writing.
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to compare.
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Makefiles and Swig files for SNR est blocks.
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an M-ary PSK signal.
This block can calculate the SNR using 1 of 4 different methods specified in the block's constructor. They (tend to) trade off accuracy for computational performnace.
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overlooked initially.
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properly (patch from Sam Bretheim).
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this forces the build system to generate these before processing the other swig files.
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to take care of it already.
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directory.
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instructions for it.
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autotools and cmake.
The autotools build does not auto-generate the Python documentation for each block like we do with the cmake build, but the empty .i files are required to build things regardless. The swig_doc.py and doxyxml files are distributed with the autotools build in case someone wants to generate this on their own (see README.doxyxml for how to do this).
Only for gnuradio-core and gr-digital currently.
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work for some reason. Need to give this another look.
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install path.
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