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
Evaluating Your Measurement Results
14
Agilent E5505A User’s Guide 339
.
To list the marked spurs
A list of spurs can be displayed by accessing the Spurs List function in the
View menu.
Forest of spurs
A so called forest of spurs is a group of closely spaced spurs on the phase noise
plot. A forest of spurs is often caused by improper shielding that allows stray
RF energy to be picked up by the DUT wiring, etc. A breadboarded or
prototype circuit should be well shielded from external RF fields when phase
noise measurements are being made.
Table 54 shows actions to take to eliminate spurs.
Table 53 Spurs on the graph
Offset Frequency Number of Averages Upward Change for Marking Spurs (dB)
<
100 kHz
<
430
≥
417
≥
812
≥
30 6
>
100 kHz Any 4
Table 54 Actions to eliminate spurs
Spur Sources Description Recommended Action
Internal Potential spur sources within the
measurement system include the phase noise
system, the DUT, and the reference source.
Typical system spurs are –120 dBc, and they
occur at the power line and system vibration
frequencies in the range of from 25 Hz to 1
kHz, and above 10 MHz.
If you do not have a plot of the system’s noise and spur
characteristics, perform the system Noise Floor Test. If
you suspect that the DUT or the reference source may
be the spur source, check each source using a
spectrum analyzer or measuring receiver (such as an
Agilent 8902A). Also, if additional sources are available,
try exchanging each of the sources and repeating the
measurement.
External Spur sources external to the system may be
either mechanical or electrical. When using
the Phase Lock Loop measurement technique,
the system’s susceptibility to external spur
sources increases with increases in the Peak
Tuning Range set by the VCO source.
Shorten coaxial cables as much as possible
(particularly the Tune Voltage Output cable). Make sure
all cable connections are tight. It may be possible to
identify an external spur source using a spectrum
analyzer with a pick-up coil or an antenna connected to
it.