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Документ взят из кэша поисковой машины. Адрес
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: http://www.naic.edu/~phil/rfi/rdr/aerostat/tpvstm_oct04.html
Дата изменения: Fri Apr 25 02:22:46 2014 Дата индексирования: Mon Apr 11 23:46:03 2016 Кодировка: Поисковые слова: annular solar eclipse |
The aerostat is a tethered balloon radar that flies above lajas puerto and is used for drug interdiction (more info).
On 06oct04 data was taken with the radar interface (RI) using pixel 2a,2b of the alfa receiver. The band was centered at 1410 Mhz. The control room front panel outputs were passed thru attenuators (pix2a 15db, pix2b 0b) and then the 300 Mhz band was detected with a 20 usecond time constant. The detected signal was then sampled at 10 usecond sampling for 48 seconds. During the data taking, the telescope was parked at az=270, za=1.9 degrees.
The attenuated version was to let us see an
unclipped
version (in the A/D's) of the radar signal when it pointed at the
AO.
The unattenuated version was to see detail when the radar was not
pointed
directly at us. These plots can be used as a reference when
someone is
looking at a square law detected signal on the oscilloscope
in the
control room. This data set includes all the radars in the 300 Mhz
band.
The discussion below is limited to the aerostat radar.
The plots show the
300
Mhz detected band versus time (.ps) (.pdf)
: