Recently I had the idea to improve the possibility to quick measure the frequency difference of two reference oscillators , in this case two Rubidium Oscillators : a Rhode Schwarz and an M100 that I put into a yellow rack with a power supply , as in the pictures .
The method is based on :
A) Multiplying by 100 the frequency of both oscillators ( with the use of simple home made Comb Generators )
B) Comparing the frequency of the two oscillators with the method of the " beats " at 1 GHz , using a selective receiver . In the test I have used a Spectrum Analyzer , but every simple receiver , even an RTL Dongle can be used with the same results .
The two Comb Generator needed was made with two EX-OR fast ports ( ACT86) , with one of the two inputs connected directly and the second through a variable resistor that , with the input capacitor of the port ,add a small delay .
The drawings can be found here : http://air-radiorama.blogspot.com/2021/02/double-symmetrically-comb-generators.html
The input is so a very sharp pulse depending on the rise and fall time of the EX-OR and of the delay of the RC constant ( in the range of ns ) .
Trimming the resistor the component at 1 GHz was at a comfortably level of -50 dBm .
The output of the two Comb generator was summed simply with two capacitor and two resistors .
You can find here the images of the output of a single Comb Generator , wide band and relatively narrow band .
What can we espect from this setup while summing the signal of the two Comb Generator at 1 GHz coming from the two Rubidium ?
The composition of the two signals will change from a maximum of +3 dB when the phase of the two oscillator is the same and to a minimum ( if the signals are exactly equal of ) zero .
In this case the spread is around 20 dB , but doesn't matter because we have only to count the cycles .
The maximums will be always very wide , while the nulls will be always very sharp .
To check this I have tuned the Rubidium M100 as far as was possible , and you can see in the first part of the following screen with zero span ( this means that the Spectrum Analyzer acts as a receiver tuned at 1 GHz with vertical logaritmic scale ) .
Please note that the horizontal time sweep is 1000 s ( 100 second/div) .
At the beginning you can count around 10 oscillations in 100s , that means one cicle each 10 seconsd = 0,1 Hz of difference at 1 GHz .
Being 1 GHz = 10E9 Hz , this means a frequency maximun difference of 10E-10 .
While time was running , I have changed the frequency of the Rubidium M100 to approach that one of the RS Rubidium .
At the end of the screen the difference is around one cycle each ten second at 1 GHz , that means 10E-11.
Continuing the approach of the frequencies , I have increased the timebase till 6000 s because the phase change was very slow .
At the end , using sequential methof of approximation , in the last picture ,it is not easy if impossible to see a real periodicity in the phase rotation and so in the frequency difference .
We are in the range of 10E-12 . I am pretty sure that this limit doesn't depend from the method of measurement ( being a "physical method ") , but from the limit of stability ( jitter ) of one ( if not both ) Rubidium Oscillator , and this was the scope of the experiment .
If I am right , this simple setup , that everyone can easily reproduce at low cost , can measure stability higher than that of Rubidium Oscillators .
To check this with no dubts , I need two oscillator with performance 10 times better than the rubidium oscilllator I have used .
Hope one day I can check this , if I am so crazy to invest in two Masers , because actually I am only playing to infringe my limits .....
But I have another couple of Rubidium Oscillators from Stanford that I can try to check in the same way ....
Claudio,
RispondiEliminail tuo post è veramente molto interessante perchè con la moltiplicazione velocizza la comparazione di fase fra gli oscillatori e soprattutto ne riporta l'andamento direttamente in forma grafica sull'analizzatore di spettro.
Idea molto bella che proverò certamente!