Age | Commit message (Collapse) | Author |
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offset), omega relative limit, and modulation order.
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but it makes the build output so much nicer...
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test sequence.
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parameter better.
The block now holds state between calls to work for the number of output symbols instead of requiring a certain number of available outputs (that may never be satisfied).
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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