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

AM Noise Measurement Fundamentals
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Agilent E5505A User’s Guide 291
Calibration and Measurement General Guidelines
• The AM detector must be well shielded from external noise especially 60 Hz
noise. The components between the diode detector and the test system
should be packaged in a metal box to prevent RFI interference.
Also, the AM detector should be connected directly to the test system if
possible, to minimize ground loops. If the AM detector and test system must
be separated, semi-rigid cable should be used to keep the shield resistance
to a minimum.
• Although AM noise measurements are less vulnerable than residual
phase-noise measurements to noise induced by vibration and temperature
fluctuation, care should be taken to ensure that all connections are tight
and that all cables are electrically sound.
• The output voltage monitor on the AM detector must be disconnected from
digital voltmeters or other noisy monitoring equipment before noise
measurement data is taken.
• The noise floor of the detector may degrade as power increases above +15
dBm. Noise in the region of the detector is best measured with about +10
dBm of drive level. The noise floor is best measured with about +20 dBm of
drive level.
• An amplifier must be used in cases where the signal level out of the DUT is
too small to drive the AM detector or is inadequate to produce a low enough
measurement 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 test
setup to avoid noise floor degradation.
• It should have only enough gain to get the required signal levels. Excess gain
leads to amplifiers operating in gain compression, increasing their
likelihood of suppressing the AM noise to be measured.
• The amplifier’s sensitivity to power supply noise and the supply noise itself
must both be minimized.
NOTE
Read This The following general guidelines should be considered when setting up and
making an AM-noise measurement
NOTE
The internal detectors in the N5500A Option 001 and N5507A, along with the 70429A
Option K21 provide this level of protection.
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