Has anyone else done this or similar
experiment?
Feb 1-2012
I did an experiment today to see
just how small an antenna I could be use to detect the hydrogen line
at 21cm.
I used three antennas for this experiment
today.
A horn (0.98m x 0.77m mouth)....
a double quadloop with "cake box lid" reflector
and....
a simple dipole with a single wire
reflector.
The ULNA I used was from Radio
Astronomy Supply. ( 0.32dB NF), 25
meters long RG-213 coaxial cable (with N-type connectors) run to the
house, then first a 21cm bandpass filter to do away with cellphone
interference, a second low noise LNA, and then two MAR-6 MMIC's
to make up for filter/cable/connector loss and to get get a decent level to
feed my HP spectrumanalyzer (@ -60dBm).
The analyzer was set for 10kHz BW and video
filtering at max, scan time at lowest speed (aprx 2min/MHz)
it's YIG frequency oscillator is
"free running" so the scan frequency is not excactly centered at 1420.5MHz
, but one can clearly see the hydrogen line around the middle of
chart..
The spectrum scan plots were done with the
spectrum analyzer D.C. vertical log output going to a dual TL-082 op amp
for level offset seting and filtering ( 2,2M Ohm to 1uF cap)+ 10X
amplification, feeding my LabJack 12 bit A/D converter, then the data
output USB goes to my 3.4GHz tripplecoare PC running Radio Skypipe
chart recorder under 'Windows 7.
Scanplot: Each scanplot shows 100kHz
horizontal division starting frfom the left at 1420.0MHz and ending at the
right at 1421.0MHz. and vertical divisions are dB/volt.
All antennas were pointed straight up towards
zenith (+ 60 Dec at my latitude). The gain was adjusted so the background
noise level showed appx -60dBm +/- 0.1 dB @ 1420.0MHz before
each scan.
As a reference level (around -60dBm is displayed as
0 dB on radio Skypipe chart) I pointed each antenna
towards coldsky @ 1420.0MHz.
Below are the results:
Even a simple dipole could detect the hydrogen line, but the
signal was burried in the noise, so one needs to filter and average
whole lot.
Even though these simple antennas (except the horn
antenna) pick up alot of hydrogen spinn/flipp photons from a very large area of
the sky, it also picks up alot of ground noise from the ground, buildings, trees
etc.
The hydrogen profiles you are used to seeing are
now more or less smeered out over a wide bandwith, so much fine
detail is lost, and averaged out, so you tend to get a bellshape profile
centered around 1420.4MHz (bad news if you want to do a sky
survey). This is due to the extreme wide
main antenna lobe.
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