User`s guide
Table Of Contents
- Title Page
- Contents
- Getting Started
- Introduction and Measurement
- Phase Noise Basics
- Expanding Your Measurement Experience
- Starting the Measurement Software
- Using the Asset Manager
- Using the Server Hardware Connections to Specify the Source
- Setting GPIB Addresses
- Testing the 8663A Internal/External 10 MHz
- Testing the 8644B Internal/External 10 MHz
- Viewing Markers
- Omitting Spurs
- Displaying the Parameter Summary
- Exporting Measurement Results
- Absolute Measurement Fundamentals
- Absolute Measurement Examples
- Residual Measurement Fundamentals
- What is Residual Noise?
- Assumptions about Residual Phase Noise Measurements
- Calibrating the Measurement
- Measurement Difficulties
- Residual Measurement Examples
- FM Discriminator Fundamentals
- FM Discriminator Measurement Examples
- AM Noise Measurement Fundamentals
- AM Noise Measurement Examples
- Baseband Noise Measurement Examples
- Evaluating Your Measurement Results
- Advanced Software Features
- Reference Graphs and Tables
- Approximate System Noise Floor vs. R Port Signal Level
- Phase Noise Floor and Region of Validity
- Phase Noise Level of Various Agilent Sources
- Increase in Measured Noise as Ref Source Approaches DUT Noise
- Approximate Sensitivity of Delay Line Discriminator
- AM Calibration
- Voltage Controlled Source Tuning Requirements
- Tune Range of VCO for Center Voltage
- Peak Tuning Range Required by Noise Level
- Phase Lock Loop Bandwidth vs. Peak Tuning Range
- Noise Floor Limits Due to Peak Tuning Range
- Tuning Characteristics of Various VCO Source Options
- 8643A Frequency Limits
- 8644B Frequency Limits
- 8664A Frequency Limits
- 8665A Frequency Limits
- 8665B Frequency Limits
- System Specifications
- System Interconnections
- PC Components Installation
- Overview
- Step 1: Uninstall the current version of Agilent Technologies IO libraries
- Step 2: Uninstall all National Instruments products.
- Step 3: Install the National Instruments VXI software.
- Step 4: Install the National Instruments VISA runtime.
- Step 5: Install software for the NI Data Acquisition Software.
- Step 6: Hardware Installation
- Step 7. Finalize National Instruments Software Installation.
- Step 8: System Interconnections
- Step 9: Install Microsoft Visual C++ 2008 Redistributable Package use default settings
- Step 10: Install the Agilent I/O Libraries
- Step 11: Install the E5500 Phase Noise Measurement software.
- Step 12: Asset Configuration
- Step 13: License Key for the Phase Noise Test Set
- Overview
- PC Digitizer Performance Verification
- Preventive Maintenance
- Service, Support, and Safety Information
- Safety and Regulatory Information
- Safety summary
- Equipment Installation
- Environmental conditions
- Before applying power
- Ground the instrument or system
- Fuses and Circuit Breakers
- Maintenance
- Safety symbols and instrument markings
- Regulatory Compliance
- Declaration of Conformity
- Compliance with German noise requirements
- Compliance with Canadian EMC requirements
- Service and Support
- Return Procedure
- Safety and Regulatory Information
286 Agilent E5505A User’s Guide
11
AM Noise Measurement Fundamentals
AM-Noise Measurement Theory of Operation
Basic noise measurement
The E5500A phase noise measurement software uses the following process to
measure carrier noise by:
• Calibrating the noise detector sensitivity.
• Measuring the recovered baseband noise out of the detector.
• Calculating the noise around the signal by correcting the measured data by
the detector sensitivity.
• Displaying the measured noise data in the required format.
Given a detector calibration, the system looks at the signal out of the detector
as just a noise voltage which must be measured over a band of frequencies
regardless of the signal’s origin.
The detector calibration is accomplished by applying a known signal to the
detector. The known signal is then measured at baseband. Finally, the transfer
function between the known signal and the measured baseband signal is
calculated.
Phase noise measurement
In the case of small angle phase modulation (<0.1 rad), the modulation
sideband amplitude is constant with increasing modulation frequency. The
phase detector gain can thus be measured at a single offset frequency, and the
same constant will apply at all offset frequencies.
• In the case of calibrating with phase modulation sidebands, the system
requires the carrier-to-sideband ratio and the frequency offset of the
sidebands. The offset frequency is equal to the baseband modulation
frequency. The ratio of the baseband signal voltage to the
carrier-to-sideband ratio is the sensitivity of the detector.
• In the case of calibrating with a single-sided spur, it can be shown that a
single-sided spur is equal to a PM signal plus an AM signal. The modulation
sidebands for both are 6 dB below the original single-sided spur. Since the
phase detector attenuates the AM by more than 30 dB, the calibration
constant can be measured as in the previous case, but with an additional
6 dB correction factor.