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

340 Agilent E5505A User’s Guide
14
Evaluating Your Measurement Results
Small angle line
Caution must be exercised where
L(f)
is calculated from the spectral density
of the phase modulation
S
φ
(f)
/2 because of the small angle criterion. Refer to
Figure 271. Below the line, the plot of
L(f)
is correct; above the line,
L(f)
is
increasingly invalid and Sf(f) must be used to accurately represent the phase
noise of the signal. To accurately plot noise that exceeds the small angle line,
select the Spectral Density of Phase Modulation (dB/Hz) graph type (
S
φ
(f)
).
L(f)
raises the noise floor by 3 dB.
The –10 dB per decade line is drawn on the plot for an instantaneous phase
deviation of 0.2 radians integrated over any one decade of offset frequency. At
approximately 0.2 radians, the power in the higher order sideband of the
phase modulation is still insignificant compared to the power in the first order
sideband. This ensures that the calculation of cal L(f) is still valid.
Electrical Electrically generated spurs can be caused by
electrical oscillation, either internal or
external to the measurement system. The list
of potential spur sources is long and varied.
Many times the spur will not be at the
fundamental frequency of the source, but may
be a harmonic of the source signal. Some
typical causes of electrical spurs are power
lines, radio broadcasting stations, computers
and computer peripherals (any device that
generates high frequency square waves), and
sum and difference products of oscillators
that are not isolated from one another in an
instrument such as a signal generator.
The frequency of the spur and patterns of multiple
spurs are the most useful parameters for determining
the source of spurs. The spur frequency can be
estimated from the graph, or pinpointed using either
the Marker graphic function which provides a
resolution of from 0.1% to 0.2% or by using the spur
listing function.
Mechanical Mechanically generated spurs are usually at
frequencies below 1 kHz. The source of a
mechanically generated spur is typically
external to the measurement system.
Try turning off or moving fans, motors, or other
mechanical devices that oscillate at a specific
frequency. (Temporarily blocking the airflow through a
fan may alter its speed enough to discern a frequency
shift in a spur that is being caused by the fan.)
Table 54 Actions to eliminate spurs (continued)
Spur Sources Description Recommended Action