Not wanting to sound like too much of a dinosaur, but back in the 1960's and
early 70's, emission data was acquired by slowly tuning a receiver across
the frequency range while listening to headphones and watching a meter. You
would record the frequency and amplitude at several frequencies per octave,
or more if you were feeling charitable, and also record any uniquely
"interesting" emission peaks. When you were finished acquisition, you might
have several pages of tabular data (perhaps 75-100 frequency / amplitude
data pairs).

 

Then, you could go back to your desk and break out your correction data, a
set of graphs for each of the parameters of cable loss, gain flatness,
bandwidth variation, pre-amplifier gain, antenna factors and maybe filter
attenuation (nothing was flat in those days). Typically, you might have 5 of
these variables, so that meant writing down (5 x 75) 375 numbers on your
data sheet. Then, you added up the raw amplitude and all factors for each
frequency and entered that corrected amplitude. Next, you used the limit of
the standard to visually interpolate and enter a limit value for each
measurement frequency. And lastly, you compared the amplitude value to the
limit value, and entered the over-limit values if necessary. And, if this
was a very formal test, you often had to break out that old pre-printed
multi-cycle logarithmic graph paper and plot the corrected data and the
limit.

 

Data correction took as long, or longer, than data acquisition. I dread to
think of the error budget!

 

The first automation that I encountered was a box using a variable speed
motor and a flexible speedometer cable connected to the tuning knob of a
receiver. You would set a "reasonable" scanning speed and connect an analog
plotter to plot detector amplitude versus scan progress (or the Volts/MHz
receiver output if you had a very advanced receiver). In this case, you
would make a master plot with a derived limit (as Ken Javor described), then
make photocopies of that master for the working measurement plots.

 

We have come a very long way in 40 years.

 

Ed Price
WB6WSN
Chula Vista, CA USA



 

From: Ken Javor [mailto:[email protected]] 
Sent: Tuesday, February 23, 2016 5:13 PM
To: [email protected]
Subject: Re: [PSES] Spectrum analyzer and noise floor

 

I agree.  A modern machine adjusts the raw data or noise floor for any and
all transducer/amplifier/attenuator factors, and if the transducer factor is
not flat, neither will be the adjusted noise floor.

The only reason we do things this way is an "embarrassment of riches" in
processing power.  Absent a digital controller, the sane way to take data
would be to adjust the limit for the transducer factors and arrive at an
adjusted limit in terms of dBuV, or dBm.  Consider the number of
computations involved in adjusting a thousand data points across a screen
for the transducer factors, vs. a simple flat or log-linear limit and
transducer factors that only need be reentered at the next frequency at
which they have changed by some set amount from the last frequency, such as
1 dB, or 0.5 dB. The adjusted limit represents orders of magnitude less
computation, plus one can reverse engineer an adjusted limit if one knows
the transducers in use, whereas adding factors to a signal above noise
renders this impossible.

Ken Javor
Phone: (256) 650-5261



  _____  

From: "McDiarmid, Ralph" <[email protected]>
Reply-To: "[email protected]"
<[email protected]>
Date: Tue, 23 Feb 2016 16:42:47 -0800
To: <[email protected]>
Subject: Re: [PSES] Spectrum analyzer and noise floor

I would like to explain to a colleague why the noise floor on a SA does not
look flat as it sweeps across a given frequency range after antenna factors,
cable factors, external gain and external attenuation are programmed into
its display function.  

I think it breaks down to these fundamental points: 

1. the SA receiver has noise in its attenuator, mixer and filter circuits
(say -80 dBm, and maybe flat within a limited  frequency range) 
2. the external amplifier has some noise too, but its gain lowers the noise
floor created by #1  (also flat within a limited frequency range) 
3. the cables have losses which are frequency dependant, and those can be
entered as loss factors into the SA  (shapes the noise floor a little and
those losses raise the noise floor) 
4. the antenna has a gain which is frequency dependant with several dB of
hills and valleys across its usable frequency range (that really shapes the
noise floor more than 1, 2 or 3 above) 
5. noise floor shape caused by #4 is the mirror image of the antenna factor
vs frequency 

Is that a decent summary? 
. 
Ralph McDiarmid
Compliance Engineering
Residential/Commercial
Solar Business
Schneider Electric D  +1 (604) 422 2622 x62622 

E  [email protected]
<mailto:[email protected]>
<mailto:[email protected]> 3700 Gilmore Way
Burnaby
BC
Canada 

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http://product-compliance.oc.ieee.org/ can be used for graphics (in
well-used formats), large files, etc.

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