Changed data logging significantly, in that for continuum data, the data
authormleech <mleech@221aa14e-8319-0410-a670-987f0aec2ac5>
Wed, 4 Oct 2006 14:36:13 +0000 (14:36 +0000)
committermleech <mleech@221aa14e-8319-0410-a670-987f0aec2ac5>
Wed, 4 Oct 2006 14:36:13 +0000 (14:36 +0000)
commitc7be5804b32bcf19739297b04f3d811bee1a47fb
tree2d1d5f6f91a19e45534095cb26e3daea30d49e45
parent58d96ee6c7c8992eaf9659668cc70530ef2f3171
Changed data logging significantly, in that for continuum data, the data
  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
gr-radio-astronomy/src/python/local_calibrator.py
gr-radio-astronomy/src/python/ra_fftsink.py
gr-radio-astronomy/src/python/ra_stripchartsink.py
gr-radio-astronomy/src/python/usrp_psr_receiver.py
gr-radio-astronomy/src/python/usrp_ra_receiver.py