Tektronix CSA8000B, TDS8000B B-24 CSA8000B & TDS8000B User Manual

Appendix B: Automatic Measurements Reference
B-24 CSA8000B & TDS8000B User Manual
Table B- 4: RZ Measurements - Amplitude (cont.)
Name Definition
RZ Q Factor A figure of merit of an eye diagram, reporting the ratio between the amplitude of the RZ pulse to
the total RMS noise on the High and Low levels. The RZ pulse 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 pulse, respectively. The noise levels are
characterized by σhigh and σlow, the standard deviations from the mean for the High and Low
levels.
Where:
HHigh and Low are the logical 1 and 0 levels.
Hσhigh and σlow are the standard deviations.
The Eye Aperture is adjustable and defaults to 5% of the RZ pulse width. See RZ Eye Aperture
Parameters on B--62.
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:
HPerform 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.
HOptimize the vertical resolution before taking this measurement. See How to Optimize the
Vertical Resolution on page B--70.
RZ Q Factor =(High −Low)
(σhigh +σlow)
RZ RMS The true root mean square of the waveform that is sampled within the measurement region.
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:
HPerform 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.
HOptimize the vertical resolution before taking this measurement. See To Optimize the
Vertical Resolution on page B--69.