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author | jcorgan | 2006-08-03 04:51:51 +0000 |
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committer | jcorgan | 2006-08-03 04:51:51 +0000 |
commit | 5d69a524f81f234b3fbc41d49ba18d6f6886baba (patch) | |
tree | b71312bf7f1e8d10fef0f3ac6f28784065e73e72 /gr-radio-astronomy/src/python/usrp_ra_receiver.help | |
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Houston, we have a trunk.
git-svn-id: http://gnuradio.org/svn/gnuradio/trunk@3122 221aa14e-8319-0410-a670-987f0aec2ac5
Diffstat (limited to 'gr-radio-astronomy/src/python/usrp_ra_receiver.help')
-rw-r--r-- | gr-radio-astronomy/src/python/usrp_ra_receiver.help | 90 |
1 files changed, 90 insertions, 0 deletions
diff --git a/gr-radio-astronomy/src/python/usrp_ra_receiver.help b/gr-radio-astronomy/src/python/usrp_ra_receiver.help new file mode 100644 index 000000000..45a21e297 --- /dev/null +++ b/gr-radio-astronomy/src/python/usrp_ra_receiver.help @@ -0,0 +1,90 @@ +This program is used to take spectra and total power measurements. + It records spectral and total-power data to external datalogging + files. + +The program takes the following options: + + --rx-subdev-spec which USRP Rx side? A or B + + --decim USRP decimation rate: 8, 16, 32, and 64 are good + (8Mhz, 4Mhz, 2Mhz, and 1Mhz bandwidth) + + --freq USRP daughtercard frequency + + --observing Actual observing frequency (default is to use the + setting for --freq) + + --avg Averaging setting for spectral display--higher numbers + equal more averaging. 25 to 40 is typical. + + --integ Total power integration time: seconds + + --gain USRP daughtercard gain control + + --reflevel Reference level on pulse profile display + + --longitude Observer longitude: West is negative + + --latitude Observer latitude: South is negative + + --fft_size Size of FFT for post-detector spectrum: default is 1024 + + --prefix Filename prefix to use for data logging files + Default is ./ + + --divbase The base of the Y/Div menu in pulsar display + + --division The initial Y/Div in pulsar display + + --ylabel Y axis label + + --cfunc The function name prefix for the spectral and + calibrator functions + + --waterfall Use waterfall, rather than regular spectral display + NOT TESTED IN THIS APPLICATION + + --stripsize Size of the total-power stripchart, in samples + +There are two windows--a spectral window, and the total-power window. + Moving the cursor around in the spectral window shows you the + corresponding frequency and doppler shift. Left clicking in this + window sets an interference marker, which sets a "zero" in the + interference filter. Use the "clear interference" button to clear this. + +The total power window is updated at a fixed 2Hz rate, and grows from + the left of the display. + +If latitude and longitude are set correctly, and system time is correct, + then the current LMST is displayed, updated once per second. + +Averaging parameters, gain, and frequency can all be set from the GUI using + the appropriate controls. You can also enter the current declination, which + will appear in the datalogging files. This is useful both for mapping, + and housekeeping purposes, particularly when you haven't looked at a datafile + for quite some time. + +There are two datalog files produced by this program: + + YYYYMMDDHH.tpdat Total power data + + The date/time portion of the filename is referred to local time, + rather than UTC or sidereal. + + First field is sidereal time when sample was taken + Second field is total power datum + Third field is declination in decimal degrees + + Samples are written once per second + + YYYYMMDDHH.sdat Spectral data + + The date/time portion of the filename is referred to local time, + rather than UTC or sidereal. + + First field is sidereal time when spectrum was taken + Second field is declination in decimal degrees + Third field is complex spectral data--in the same order that FFTW3 library + places bins: DC to bandwidth/2, followed by -bandwidth/2 to DC. + + Spectral snapshots are written once every 5 seconds |