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Data Analysis and Preliminary Results
Development of a Cleanliness Specification
for Expanded Beam Connectors: Phase II
Dr. Michael A. Kadar-Kallen
Senior Principal Engineer
iNEMI meeting, March 12th at OFC 2018
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.12 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.12
A Proposed Cleanliness Specification forExpanded Beam Connectors
The cleanliness of a lensed surface is quantified by:
Specifying the intensity distribution at the lensed surface
Measuring the distribution of dust on this surface
Calculating the loss
The Calculated Loss is compared to an Acceptable Loss Limit to determine whether a dusty lens
“passes” or “fails”.
This can be easily incorporated into existing connector inspection equipment, which can generate
both a pass/fail message and the Calculated Dust Loss
Calculation of the Dust Loss
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.14 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.14
Multimode Dust Loss Calculation
The multimode dust loss* is calculated based on two inputs:
• The distribution of dust particles: D(x,y)
• The distribution of light: I(x,y)
This Calculated Loss is strongly correlated with the Measured Loss. The Calculated Loss is nearly
identical to the Simulated Loss determined by optical modeling.
* All three types of loss (Measured, Calculated, Simulated) refer to the “dust loss”,
the additional loss caused by the presence of dust.
D(x,y) I(x,y)
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.15 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.15
The intensity distribution at the lens surface is approximated by a quadratic function of radius:
Note: this is the intensity distribution at the endface of a graded-index multimode fiber with
Over-Filled Launch conditions
A quadratic function is a reasonable, simple approximation to the
Over-Filled and Encircled Flux intensity distributions at the lens surface
The diameter (2a) of the expanded beam of the
PRIZM® MT is approximately 200 µm
Intensity Distribution
otherwise0
0/1),(
2arar
arI
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.16 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.16
Calculating the Dust Loss: Image Processing
I(x,y) D(x,y) I(x,y)D(x,y)
dxdyyxI
dxdyyxDyxIT
),(
),(),(MM Dust,
Sum over all pixelsSum over all pixels
X =
Calculated
Intensity
Distribution
Measured Dust
Distribution
Intensity
Distribution
Obscured by Dust
Preliminary Results
Data taken February 26-27, 2018 by US Conec and FiberQA
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.18 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.18
Repeatability
The repeatability of the Measured and Calculated Loss was measured before the main experiment,
for both clean and contaminated samples, with and without re-mating between measurements.
In hindsight, the contaminated sample is not ideal.
The lenses have either too much (> 1 dB) or too little (<0.1 dB) contamination.
10 sets of 12 images were taken before and 8 after the test
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.19 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.19
Repeatability Images (Raw and Processed): First 3 Sets
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.110 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.110
Repeatability Analysis of the Calculated Loss of Contaminated Lenses before the Experiment
High variability for samples with high loss No data
between 0.1 and 1.0 dB
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.111 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.111
Repeatability Summary
Measured Loss, Pre-Test
A - Clean, no re-mating, first sample: 6σ = 0.013 dB
B - Clean, no re-mating, second sample: 6σ = 0.018 dB
C - Clean, with re-mating, second sample: 6σ = 0.028 dB
D - Contaminated, with re-mating, second sample: 6σ = 0.20 dB
Measured Loss, Post-Test
E - Clean, no re-mating, first sample: 6σ = 0.016 dB
F - Contaminated, with re-mating, second sample: 6σ = 0.21 dB
Calculated Loss, Pre-Test
D - Contaminated, re-mating: 6σ = 1.8 dB
Calculated Loss, Post-Test
F - Contaminated, re-mating: 6σ = 0.5 dB
Note: The quantization error for a meter with 0.01 dB resolution is: 6σ = 0.017 dB
99.7% of measurements fall within ±3σ of the average
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.112 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.112
Experiment: Measured and Calculated Loss
ImageMeasure
IL (1)Image
Add Dust
DUT
N
ImageMeasure
IL (2)Image
Change
Contamination?
NoYesAdd or Remove
Dust
DUT
N+1
Note: each contaminated lens is measured only once.Every data point represents a unique distribution of dust.
Measured Loss (dB)
= IL (2) dB – IL (1) dB
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.113 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.113
Calculated vs. Measured Loss
0 – 1 dBAll Data
10 DUT
172 Independent Data Points
144 With a Measured Dust Loss ≤ 1 dB
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.114 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.114
Calculated vs. Measured Loss, with Comments
0 – 1 dBAll Data Significant scatter when the Measured Loss is above 1 dB
The Calculated Loss is above 1 dB, which signals to the user that the lens needs to be cleaned.
Less scatter below 1 dB
The Calculated Loss exceeds the Measured Loss: it is a conservative estimate of the dust loss
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.115 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.115
Calculated vs. Measured Loss
All Data
The residuals are not Normal. R2 = 0.90; 6S = 2.1 dB
Residuals are smaller when the loss is smaller
)3( 08.009.1Measured
Calculated
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.116 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.116
Data with Measured Dust Loss ≤ 1 dB
Measured Dust Loss ≤ 1 dB
The residuals are Normal. R2 = 0.97; 6S = 0.7 dB
Residuals are smaller when the loss is smaller
)3( 06.049.1Measured
Calculated
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.117 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.117
Setting the Calculated Loss Limit – An Example
In this example, the goal is to keep the actual (measured) dust loss less than 0.5 dB.
We set the pass/fail limit for the Calculated Loss at 0.5 dB, so that no dirty parts are accepted.
30% of the time, a clean part is rejected.
Even though the data is noisy and the pass/fail limit is biased to avoid accepting dirty parts, the correct decision is made 70% of the time.
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.118 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.118
Conclusions
• As in the Phase I experiment the Calculated Loss is correlated with the Measured Loss
• The repeatability of the Calculated Loss is not as good as hoped
• This appears to be due to focusing errors that were not noticed during data collection, which is in turn due to the unusually large thickness of the contaminants
• The repeatability improves significantly at lower losses. At zero loss (no dust particles) the repeatability of the Calculated Loss is perfect!
• Even with this noisy data, it is possible to set a pass/fail limit on the Calculated Loss such that:
• No dirty parts are accepted
• Most parts are correctly identified as clean or dirty
• The Calculated Loss is a quick, simple measure of contamination by dust
These are preliminary results. The experiment started 2 weeks ago today. Changes to the image
analysis may improve the results.
PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc. | v1.120 PRIVATE AND CONFIDENTIAL © 2017 CommScope, Inc | v1.120
In the absence of dust, the power in a beam of light is the integral of the intensity distribution
over a surface that is perpendicular to the optical axis:
We define the dust transmissivity as
The fraction of the power transmitted by a dusty surface is
In a low-loss multimode system, all of the power that is transmitted through the dusty surface is
coupled into the receiving fiber or detector:
Calculated Dust Transmission
dxdyyxIdAIP ),(
otherwise1
present isdust where0),( yxD
dxdyyxI
dxdyyxDyxIT
),(
),(),(MM Dust,
MM Dust,10MM Dust, log10(dB)IL T
Circular Dust Particle BlocksRays of Light in a Zemax Model
Dust