Miscellaneous devices
Links to different devices:
axis 212 ptz web camera.
Axis 212 ptz web camera:
Sections:
17oct06: looking at the birdies in
the shielded room.
17oct06: rfi from the axis 212 camera seen through
the telescope.
Summary:
Plots:
The
325 and 324 Mhz birdies in the shielded room (.ps) (.pdf)
Average
of (camera on)/(camera off) - 1 (on the telescope) (.ps)
(.pdf
)
Dynamic spectra:
324
Mhz dynamic spectra: camera in the parking lot (.gif):
324
Mhz dynamic spectra: camera in the control room (.gif):
325
Mhz dynamic spectra: camera in the parking lot (.gif):
325
Mhz dynamic spectra: camera in the control room (.gif):
An axis
212ptz web cam is to be installed in the control room and at
the visitor center in oct06. We checked for rfi emissions in the shielded
room and on the telescope. When we made the measurements, the ethernet
was not connected.
17oct06: looking at the birdies in
the shielded room.
The rfi output of the camera was measured in the shielded
room on 17oct06 using the ybt250 (Tektronix) spectrum analyzer. The
small loop antenna was placed close to the lens of the camera and rotated
to give maximum signal.
We found a comb with a 25 Mhz spacing sitting
at 300,325,350 etc. Mhz. The comb elements seem to be modulated with about
a 100 Khz bandwidth. T
I stepped through 100 Mhz to 1500 Mhz with a 100
Mhz span and then came back and looked at some of the comb elements with
a higher resolution (note: RBW is resolution band width). A list of some
of the more prominent birdies are:
| freq |
rbw |
amp (db) |
Notes |
| 323.997 |
100 Hz |
32 |
Very narrow |
| 325 |
10 Khz |
25 |
about 100 Khz fwhm |
| 347.996 |
100 Hz |
32 |
very narrow |
| 375 |
100 Khz |
20 |
100 Khz fwhm |
| 400 |
100 Khz |
15 |
|
| 425 |
1 Khz |
10 |
|
| 675 |
1 Khz |
15 |
The adjacent noise floor moves down by 15 more db when the camera is
off. |
700
725 |
30 Khz |
25 |
100 Khz wide birdie |
775
800 |
1 Mhz |
20 |
|
| 1375 |
1 Khz |
20 |
adjacent 1374.9 birdie was from repeater |
More Notes:
-
The 650-800 Mhz was pretty mess. When the camera was powered off the entire
band moved down by about 15 db so there is some continuum emission.
-
Most of the birdies that sat on multiples of 25 Mhz had a FWHM of
100 Khz.
-
The narrow birdies at 323.997 and 347.996 were not resolved with the 100
Hz RBW.
Plots were made of the
325 and 324 Mhz birdies in the shielded room (.ps) (.pdf).
The data was taken with the loop antenna and the Tektronix spectrum analyzer
in the screened room:
-
Top: this is the 325 Mhz birdie. with a 10 Khz rbw. It is one of the stronger
comb elements. The black trace has been averaged by 10 sweeps, the red
trace is a peak hold.
-
Bottom: The 324 Mhz narrow birdie. The rbw was 100 hz. This narrow birdie
was also seen at 347.996 Mhz.
processing: x101/061017/cameralab.pro
17oct06: rfi from the axis 212
camera seen through the telescope.
On 17oct06 we looked at the rfi from the axis 212 camera
using the telescope. The setup was:
-
Interim correlator with 380 hz resolution (after hanning) 324 Mhz and 25
Khz resolution.
-
1 second integrations were taken. During this time we turned the camera
on and off.
-
We used the 327 Mhz receiver (Tsys about 130K) for the 324 and 325 Mhz
birdies. lbw (tsys about 28K) for the 1375 Mhz birdie.
-
The telescope was parked at az=337.2, za=19. This position gave a maximum
when we transmitted from the control room (see az,za
dependence of transmitted birdies).
-
Data was taken with the camera in the parking lot adjacent to the control
room (in the rfi van). It was also taken with the camera in the control
room on the desk next to the observer2 workstations. These were the same
two positions used for the transmitted birdies test. So hopefully the az,za
we picked was close to a maximum. The only difference would be the field
pattern of the transmit antenna versus the field pattern of the camera.
The first plots are dynamic spectra for 324 Mhz and 325 Mhz with the camera
in the parking lot and in the control room. The horizontal dashed lines
surround when the camera was turned off:
-
324 Mhz Birdie (narrow band):
-
325 Mhz Birdie (100 Khz fwhm). Part of the 25 Mhz comb.
The average
of (camera on)/(camera off) - 1 (.ps) (.pdf
) is also plotted. Black has the camera in the parking lot, red is
in the control room:
Top: 25 Khz resolution centered at 325 Mhz. The dashed green lines
are the two birdies. You see them in the parking lot but not in the control
room.
Center: 390 Hz resolution spectrum shows that the narrow band birdie
is at 323.995 Mhz. It is 1.5 times Tsys in a 390 Hz channel when the camera
is in the parking lot.
Bottom: blowup of the 390 Hz resolution spectra. You can see a small bump
in the control room (red) spectra about 1 Khz above the camera birdie.
This is probably the streak we saw in the 324 Mhz dynamic spectra from
the control room. Since the 323.995 birdie remained relatively stable,
my guess is that the birdie we saw in the control room is not coming from
the camera.
processing: x101/061017/cam_on_tel.pro
Summary:
-
The axis 212 camera has a 25 Mhz comb at multiples of 25 Mhz. It is about
100 Khz wide
-
Two narrow birdies were seen at 323.995 and 348 Mhz.
-
Some of the stronger birdies seen in the screen room were: 324,325,348,375,700,725,1375
Mhz.
-
With the camera in the parking lot we see the camera birdies at 323.995
and 325 Mhz. The 323.995 birdie is 1.5 times Tsys in a 390 Hz channel.
We do not see the birdie at 1375 Mhz.
-
With a 100 second integration the 325 and 324 Mhz birdies were not seen
in the control room.
-
If the camera is placed at the visitors center, it will have to be put
inside a shielded box.
-
If the camera is placed in the control room then you probably can use it
without a shielded box. The only question is whether there is an az,za
and camera position that will be much stronger than the ones we used. If
the rfi shielded boxes are not hard (expensive) to build, it might be a
good idea to put all of the cameras in a box.
home_~phil