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Appendix B: Automatic Measurements Reference
B- 48
CSA8000B & TDS8000B User Manual
Table B- 7: NRZ Measurements - Amplitude (cont.)
Name
Definition
NRZ Q Factor
NRZ Q Factor is a figure of merit of an eye diagram, reporting the ratio between the amplitude
of the NRZ eye to the total RMS noise on the High and Low levels. The NRZ eye is sampled
within the Eye Aperture, where the High and Low levels are determined as the mean of the
histogram of the data distribution in the upper and lower half of the eye, respectively. The noise
levels are characterized by
σ
high and
σ
low, the standard deviations from the mean for the High
and Low levels.
Where High and Low are the logical 1 and 0 levels, and
σ
high and
σ
low are the standard
deviations. See
RZ Eye Aperture Parameters
on B--62.
The Eye Aperture is adjustable and defaults to 20% of the NRZ bit time.
If enabled, measurement gates constrain the measurement region to the area between the Start
Gate (G1) and Stop Gate (G2). See
To Localize a Measurement
on page 3--83.
This measurement requires the use of a waveform database. When this measurement is turned
on, it will automatically set the measurement system to use a waveform database if available.
See
Use a Waveform Database
on page B--70.
For best results with this measurement:
H
Perform a Dark Level compensation before taking this measurement if the source of the
measured waveform is an optical channel. See
To Perform Dark-Level and User
Wavelength Gain Compensations
on page 3--98.
H
Optimize the vertical resolution before taking this measurement. See
How to Optimize the
Vertical Resolution
on page B--70.
NRZ Q Factor
=
(
High
−
Low
)
(
σ
high
+
σ
low
)
NRZ RMS
The true root mean square amplitude of the selected waveform within the measurement region.
See
Defining and displaying waveforms
on page 3--56.
If enabled, measurement gates constrain the measurement region to the area between the Start
Gate (G1) and Stop Gate (G2).
When this measurement is turned on, it will automatically set the measurement system to use a
waveform database if available.
For best results with this measurement:
H
Perform a Dark Level compensation before taking this measurement if the source of the
measured waveform is an optical channel. See
To Perform Dark-Level and User
Wavelength Gain Compensations
on page 3--98.
H
Optimize the vertical resolution before taking this measurement. See
To Optimize the
Vertical Resolution
on page B--69.
Содержание CSA8000B Series
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Страница 18: ...Preface xiv CSA8000B TDS8000B User Manual ...
Страница 26: ...Check the Package Contents 1 8 CSA8000B TDS8000B User Manual ...
Страница 62: ...Accessories and Options 1 44 CSA8000B TDS8000B User Manual ...
Страница 76: ...Overview 3 2 CSA8000B TDS8000B User Manual ...
Страница 112: ...Acquiring Waveforms 3 38 CSA8000B TDS8000B User Manual ...
Страница 126: ...Triggering 3 52 CSA8000B TDS8000B User Manual ...
Страница 146: ...Displaying Waveforms 3 72 CSA8000B TDS8000B User Manual ...
Страница 174: ...Measuring Waveforms 3 100 CSA8000B TDS8000B User Manual ...
Страница 186: ...Creating Math Waveforms 3 112 CSA8000B TDS8000B User Manual ...
Страница 214: ...Data Input and Output 3 140 CSA8000B TDS8000B User Manual ...
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