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1) Modified top-level run_tests.sh script:
a) to execute code for setting or changing the library search path in
Darwin (DYLD_LIBRARY_PATH) or Windows (PATH) on those host OSs
only, not on other host OSs.
b) Added local (to the component making check) library paths to those
same search paths, since libtool doesn't do it (unlike in Linux).
2) In all AM Makefiles -except those dealing with USRP firmware-,
changes INCLUDES to AM_CPPFLAGS since the former is deprecated.
3) Changed AM_CPPFLAGS to FW_INCLUDES for commands .c.rel in USRP
firmware.
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GNU Radio modules individually, using already installed dependent libraries and include files. New functionality is enabled using --with-* on configure command line; existing build options should remain unchanged. Nice work by Michael Dickens, still needs documentation update on wiki.
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Temporarily removed audio output.
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Added -Q (--seti_range) option to allow setting of scanning bandwidth in
SETI mode.
Added more statistical output in seti_analyser
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frequency changes.
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using --notches.
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Added bounds-checking/setting for both --calib_coeff and --calib_offset
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on the command line only, as --calib_offset and --calib_coeff. Now
you can tweak them with the GUI, and the command line options have
different scaling than previously.
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Changed usrp_ra_receiver to use dbid() method to determine which card type
is being used.
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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.
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Fixed type mistmatch in Numeric.zeros()
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This moves usrp related .py files from the top-level of site-packages
into site-packages/usrpm.
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with libtool and already installed libraries.
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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.
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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.
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bandwidth to 12.5Khz, allowing sub-1Hz resolution.
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necessitated an RA-specific version of waterfallsink.
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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.
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bandwidth, integration time, spectral averaging, and gain. This
necessitated a change to data file syntax in the last token, but the
post-processing scripts have been updated to handle both old and new
formats. In the old format, there was a single "annotation" token--
the current declination.
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run_tests.in for Python QA has been extracted into run_tests.sh in the
top-level and the individual run_tests just invoke that with the right
path parameters. Also fixed Cygwin 'make check' bug by adding fix by
Don Ward.
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Merged -r3250:3255 from jcorgan/ticket-26.
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/gnuradio/branches/developers/jcorgan/ticket-10. 'make distcheck' now
successfully completes on a machine that has never had gnuradio installed
before. In addition, several cleanups and refactoring of build system
code have been applied. NOTE: gr-audio-portaudio, gr-audio-osx, and
gr-audio-windows have not been fully tested and will need verification
by the maintainers of these components.
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appropriate.
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