STI measurements

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bobnoise
view post Posted on 15/11/2017, 15:44




Firstly, thank-you Angelo and University of Parma for putting this together, it looks like it might be exactly what I've been searching for. :)

Some questions on the STI measurement procedure:

Aurora43Manual.pdf references IEC 60268-16 (2003) although the results page now shows 2011 complaint data. IS the plugin fully complaint with 2011 results presentation requirements?

The procedure says:
Measure background noise
Measure pink noise in reciver position with level at 62dB (A) at 1m (from source) and filtered so that the specrtrum is as per the male voice spectrum.

IEC 60268-16 (2011) says to ensure the 1/3 octave bands are with +/- 1dB over the frequncy range (ie flat) using a FULL STI MLS or STIPA signal.

IEC 60268-16 (2011) says to set the source level at 60 dB (A) at 1m and does not appear to make provision for measuring pink noise and convolving using the IR to determine modulation reduction. Have you made a comparitive study between the FULL STI or STIPA method and the Aurora method?

Could you confirm that for the Aurora 4.4 plugin 60 dB (A) at 1m pink noise with a flat spectrum in octave bands is to be used?

The anticipated variation in STI values between the Aurora method and STIPA method?

thank-you
 
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view post Posted on 16/11/2017, 12:34
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Aurora43Manual.pdf references IEC 60268-16 (2003) although the results page now shows 2011 complaint data. IS the plugin fully complaint with 2011 results presentation requirements?

Yes, the module was updated in 2012 and is now fully compliant with the new version of the IEC standard. The Manual was NOT updated, indeed...

The procedure says:
Measure background noise
Measure pink noise in receiver position with level at 62dB (A) at 1m (from source) and filtered so that the specrtrum is as per the male voice spectrum.

This is not fully correct: you should make 4 RECORDINGS:
1) calibrator signal (typically 94 dB, 1 kHz, inserting the calibrator onto the microphone)
2) background noise level (source turned off)
3) signal+noise level (source turned on, fed with equalized pink noise, calibrated a 60 dB(A) at 1m and equalized properly)
4) impulse response (source turned on and at maximum power, fed with exponential sine sweep signal, without equalization).


IEC 60268-16 (2011) says to ensure the 1/3 octave bands are with +/- 1dB over the frequncy range (ie flat) using a FULL STI MLS or STIPA signal.

Again, this is not correct: please note that Aurora employs the "indirect" method as described in table 3 of the standard. What you says refers to the "direct" method, which nowadays is obsolete. For the indirect method, the standard says that the test signal should be pibnk noise equalized in such a way to have a spectrum complying with the "male" or "female" 1/3 spectra provided in the standard (table A4). It should NOT be flat! I usually equalize the sound source for the "male" spectrum, as the Aurora STI plugins already performs for you the computation applying the "male to female" spectral correction.

IEC 60268-16 (2011) says to set the source level at 60 dB (A) at 1m and does not appear to make provision for measuring pink noise and convolving using the IR to determine modulation reduction.

Yes, the new version of the standard reduced the standard calibration value of the voice-shaped spectrum to 60 dB(A) at 1.0m. Again, the manual of Aurora was not updated, sorry!
Indeed, the new version of the standard describes in detail the "indirect" method (clause 6 of the standard, "Indirect method of measuring STI using the impulse response", which was first employed in Aurora, consisting in separating the "Signal+noise" measurement, employing equalized pink noise, form the "impulse response" measurement, employing sine sweeps.


Have you made a comparitive study between the FULL STI or STIPA method and the Aurora method?

Yes, of course. Here some papers:
www.angelofarina.it/Public/Papers/180-Euronoise2003.pdf
www.angelofarina.it/Public/Papers/184-Rieter2003.pdf

And, for an independent evaluation, see here:

www.iiav.org/icsv21/content/papers...25070451775.pdf


Could you confirm that for the Aurora 4.4 plugin 60 dB (A) at 1m pink noise with a flat spectrum in octave bands is to be used?

60 dB(A) at 1m is correct, but no, the spectrum is not flat! You should adjust the spectrum using Audition's 1/3 octave band equalizer until the compiiance with the spectrum recommended by the IEC standard is obtained (Table A.4):
Table-_A4

The anticipated variation in STI values between the Aurora method and STIPA method?

It cannot be anticipated, it depends on the system being tested, but as Aurora provides both STI and STIpa you can see the difference (if any) directly on the plugin...
 
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view post Posted on 20/1/2020, 16:49

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Very interesting topic.

One question on the procedure: if I cannot measure the pink noise level at 1m from the source (to assess the 60dB(A)) but I am able to do the rest of the calibration, can i create a pink noise signal with the right value compared to dBFS and use it as my calibration file?

If yes how can I define the amplitude?

Something like this: 10(-6dBFS/20) = 0.5

thanks
 
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view post Posted on 23/1/2020, 11:17

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Some part of the new standard rely on absolute SPL correction factors, hence the answer is NO. You cannot make a calibration "realtive" to full scale, you need to calibrate your source in "absolute" dB-SPL.
However, I do not see the problem.
I usually calibrate the source at the beginning of the measurement session. I just place the SLM at 1m from the source, on axis, and I adjust the knob until I read 60 dB(A). It takes perhaps 1 minute, so what's the problem doing this?
What can be done in advance is to create the pre-equalized pink noise WAV file to be played on your specific source.
While the loudpeaker is behaving linearly, the equalization is independent on the the gain (and of consequence on the absolute SPL value).
For creating the pre-equalized pink noise WAV file you start with a flat pink noise, generate with Adobe Audition, long, say, 1 minute.
You play it and record with a microphone in front of the source, at 1m.
Make an octave-band analysis using the Aurora STI module, and copy and past the spectrum to an Excel spreadsheet.
Evaluate at each ovtave band the difference between the octave-band level and the total A-weighted level, and write these number below those mandate by the standard, and shown in the table above (for male speaker).
Of course there will be discrepancies, at some frequencies the measured value will be larger and at other frequencies the measured value will be smaller than the value in the IEC table.
At each frequency, you calculate the correction (value in the table - measured value).
These are the offsets to be applied to the pink noise wav file, using the Audition's graphical equalizer effect, set in octave-band mode.
At each frequency, move the slider (or key-in the value) of the offset computed in Excel, then hit apply.
The result will be a new WAV file containing equalized pink noise.
You can repeat the playback & recording again, for checking that now the resulting octave band spectrum is compliant with the table in the standard. If it is not, compute again the residual correction to be applied, and perform again the graphical equalization in audition.
repeat until the measurement shows a spectrum which is perfectly compliant with the IEC standard.
this WAV file will be used for feeding your loudspeaker when doing measurements. after adjusting the total A-weighted level to 60 dB(A) at the beginning of each measurement session, as explained.
 
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view post Posted on 23/1/2020, 11:49

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QUOTE
It takes perhaps 1 minute, so what's the problem doing this?

I agree with what you describe but I have to say it is not always possible to follow this procedure.
If you use your own source, this is easy to do, but if you have to measure the STI performance of a sound system in a big arena, it is not always easy to go up and put your SLM at 1m from the big line arrays.
Also I would question if your measurement at 1m from a line array is representative of the SPL @1m of the system.

So there is the need of an alternative to this in my view, as I happen to do quite a lot of this work.
 
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view post Posted on 25/1/2020, 18:26

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Probably there is some misunderstanding of the procedure...
At 1m from a powerful line array, the equalized pink noise will probably be well above 100 dB(A)!
The calibration at 60 dB(A) at 1m is for the artificial mouth. When there is a PA system the artificial mouth should be placed at a few cm from the microphone employed for the announcements.
Then the gain of the PA system is adjusted until the system delivers the contractual SPL at the reference listening position. A typical value can be something as 80 dB(A) in a listening position very far from the loudspeaker.
In venues where the microphone is inside tha same room as the loudspeakers, usually the gain is limited by the feedback.
This is not an issue when the microphone is in a separate room, so there is no feedback.
In this case, it is also possible to inject directly a dummy microphone signal in the PA system, obtained recording the signal from a typical PA microphone placed in front of the calibrated artificial mouth.
When instead the microphone is inside the venue, the use of the artificial mouth in front of the microphone is mandatory, you cannot measure STI injecting an electrical signal into the system.
 
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view post Posted on 7/10/2020, 22:51

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Hi Angelo....here's Winhay another aurora user.

I have a doubt with the STI measurements.

Specifically with impulse response for STI

I readed we can use a sweep signal with no equalization and no necessarily 62 dBA......ok, but about my source??.....

For example, can I use the impusle response used for evaluating acoustical parameters for evaluating the STI parameter?...(omnidirectional source)

or

When I measurement STI parameters I MUST obtain the IMPULSE response with a directional speaker ( emulate directionality of the male voice)


I know I'm must use a directional speaker for obtain the filter signal of the source......but If i have already the impulse response of a room
measured with a omnidirectional source it's necesary obtain the impulse response with a directional speaker?....

I hope my question can be understand

Regards
 
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view post Posted on 22/12/2020, 00:38
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Il Lato Oscuro della Fase. Divulgazione sui temi dell'Acustica applicata al Sound System Design

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For Winhay
Indirect method is based on the measurament of the IR of the room, and in the separate estimation of the spectra of the Noise and the spectra of the signal.
it depend on the Room, its dimensions and its caracteristics. If the room is not very large, you can use the vocalbox itself at maximum level (without many distortion if possible). Instead if the room is Large, i think is mandatory the use of Dodec.
The gathering of a noiseless room impulse response represents the foundation of all measures. Obtaining this signature with a standardized method that can be valid for all possible measures is the key to optimizing the work.
So I would say that you must to get the Room Impulse Response always in the best possible way. Use the dodecaedrum

Edited by FedeleDeMarco - 31/12/2020, 13:06
 
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view post Posted on 28/12/2020, 14:30

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FedeleDeMarco.

thanks! for the answer....it's very useful for me reinforce this kind of concepts......regards!
 
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view post Posted on 28/12/2020, 14:39
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Thanks to you.
read all the topics related to STI, by Prof Farina (our continuous inspiration), that you can find in the forum (also older posts).
take a look at my webinars on my Youtube Channels (often based on Farina's work):
 
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view post Posted on 31/12/2020, 12:05
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For standard-compliant measurements you should use the artificial mouth (small directive loudspeaker) both when measuring SIGNAL (with calibrated and equalized pink noise, featuring 60 dB(A) at 1m) and when measuring the Impulse Response.
In the second case, indeed, you do not need to equalize, nor to reduce the gain for getting 60 dB(A) at 1m: you can use the loudspeaker with flat response and maximum power.
 
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view post Posted on 8/11/2021, 14:49
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Hi Pr Farina,

First of all, thanks a lot for making all your tools available for anyone, I appreciate it !

I am trying to use the STI module in Audacity, so I have my 4 required tracks (calib, background, signal and IR), I perform the calibration and once I'm in the SNR Calculation tab, after selecting the background noise and signal tracks, when I click on "Compute levels" the levels do not seem correct (around -100 dB).

I also tried amplifying the signal track to see if it changes the calculated sound levels, but there is no change.

Is that normal ?

Thanks in advance for your help
 
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view post Posted on 8/11/2021, 16:08
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Can you share a sample of your 4 WAV files?
So I can check what happens with them...
I made the lesson on STI measurements this morning in my classroom, recorded with Zoom.
You can see the recording here:
http://www.angelofarina.it/Public/Acoustic...2021/zoom_4.mp4
And here you find the WAV files recorded in the classroom:
www.angelofarina.it/Public/Acoustics-Course/WAV-2021/IR-STI/
You can try to replicate my own measurement, which gave a result of STI-male=0.577, using these 4 files:
1) Calibration-68dBA-Nevaton-W.wav
2) Background-Noise-Nevaton-W.wav
3) Signal+Noise-Nevaton-W.wav
4) IR-Sweep-Bformat-W.wav
 
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view post Posted on 10/11/2021, 12:08
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Hi,
Thanks a lot for taking the time to answer. Here are the 4 files (IR still needs to be computed from Sine Sweep recording) :

drive.google.com/drive/folders/10JPh9vIboQi20S2-awWx5_CF-_ywr-vf?usp=sharing

I also included 2 pictures in that folder showing what happens when I use your recordings to compute the STI ("STI-Background-S+N.png" and "STI-calib.png").
As you can see the computed sound levels are far below 0 dB, so I'm thinking it could be a problem with the plugin?
Thanks again for your help !
Best regards
Christophe
 
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view post Posted on 13/11/2021, 10:59
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The Google Drive folder is not accessible.. I did "request access" to it...
 
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17 replies since 15/11/2017, 15:44   1451 views
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