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
210 Agilent E5505A User’s Guide
7
Residual Measurement Fundamentals
table will often knock a sensitive residual phase noise measurement out of
quadrature.
4
When making an extremely sensitive measurement it is essential to use
semi-rigid cable between the components. The bending of a flexible cable
from vibrations and temperature variations in the room can cause enough
phase noise in flexible connecting cables to destroy the accuracy of a
sensitive measurement. The connectors also must be tight; a torque wrench
is the best tool.
5
When measuring a low-noise device, it is important that the source and any
amplification, required to achieve the proper power at the phase detector,
be placed before the splitter so it will be correlated out of the measurement.
In cases where this is not possible; remember that any noise source, such as
an amplifier, placed after the splitter in either phase detector path, will
contribute to the measured noise.
6
An amplifier must be used in cases where the signal level out of the DUT is
too small to drive the phase detector, or the drive level is inadequate to
provide a low enough system noise floor. In this case the amplifier should
have the following characteristics:
• It should have the lowest possible noise figure, and the greatest possible
dynamic range.
• The signal level must be kept as high as possible at all points in the setup
to minimize degradation from the thermal noise floor.
• It should have only enough gain to provide the required signal levels.
Excess gain leads to amplifiers operating in gain compression, making
them very vulnerable to multiplicative noise problems. The non-linearity
of the active device produces mixing which multiplies the baseband
noise of the active device and power supply noise around the carrier.
• The amplifier’s sensitivity to power supply noise and the power supply
noise itself must both be minimized.
Calibration options
There are six calibration methods that to choose from for calibrating a
two-port measurement. The procedure for each method is provided on the
following pages. The advantages and disadvantages of each method are also
provided to help you select the best method for your application. The primary
considerations for selecting a calibration method are:
• Measurement accuracy
• Equipment availability