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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@6044 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@5570 221aa14e-8319-0410-a670-987f0aec2ac5
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Changed usrp_ra_receiver to use dbid() method to determine which card type
is being used.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@5564 221aa14e-8319-0410-a670-987f0aec2ac5
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gr_complex_to_mag_squared(). I'm hoping this will save a little in
terms of buffer management and CPU cycles.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@5060 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@4817 221aa14e-8319-0410-a670-987f0aec2ac5
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Fixed type mistmatch in Numeric.zeros()
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@4759 221aa14e-8319-0410-a670-987f0aec2ac5
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This moves usrp related .py files from the top-level of site-packages
into site-packages/usrpm.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@4728 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3873 221aa14e-8319-0410-a670-987f0aec2ac5
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sky at the time or not.
Increased the difficulty of the "gauntlet" that "hits" in the SETI mode
have to run through in order to be considered a hit. Hard to test :-)
Added intensity levels to SETI hit logging. This will allow post-facto
gaussian profile determination for any hits that are found.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3842 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3772 221aa14e-8319-0410-a670-987f0aec2ac5
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continuous frequency-scanning, the continuum data will be invalid
anyway, and of little use.
This saves a little bit of CPU, so I've been able to get a 25Khz
FFT with a length of 32768 bins, for continued sub-1Hz resolution,
but with a wider instantaneous bandwidth. For some reason, though,
there's a "knee" in the curve, and running at 50Khz sampling increases
the CPU consumption by a much larger factor than you'd expect.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3764 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3759 221aa14e-8319-0410-a670-987f0aec2ac5
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bandwidth to 12.5Khz, allowing sub-1Hz resolution.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3758 221aa14e-8319-0410-a670-987f0aec2ac5
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necessitated an RA-specific version of waterfallsink.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3735 221aa14e-8319-0410-a670-987f0aec2ac5
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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
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3602 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3571 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3534 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3488 221aa14e-8319-0410-a670-987f0aec2ac5
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git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3122 221aa14e-8319-0410-a670-987f0aec2ac5
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