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Keysight Q347B Q-Band Noise Source: Unleash Precision Noise Generation from 33 GHz to 50 GHz
$5,100.00
Keysight Q347B Q-Band Noise Source: Generate accurate and reliable noise signals for testing and calibration applications in the 33 GHz to 50 GHz frequency range.
Keysight Q347B Q-Band Noise Source, 33 GHz to 50 GHz
Product Overview
The Keysight Q347B Q-Band Noise Source is a high-performance noise source designed for use in a variety of applications, including radar, electronic warfare, and satellite communications. It provides a broadband, flat noise spectrum from 33 GHz to 50 GHz, making it ideal for testing and characterizing receivers and other RF components.
Features and Specifications
 Frequency range: 33 GHz to 50 GHz
 Output power: -10 dBm to -120 dBm
 Noise figure: < 15 dB
 VSWR: < 1.5:1
 Dimensions: 2.5″ x 2.5″ x 1.0″
 Weight: 1.0 lb
Benefits
 Broadband, flat noise spectrum for accurate testing of receivers and other RF components
 High output power for testing high-sensitivity receivers
 Low noise figure for minimizing noise contamination
 Compact size and lightweight for easy portability
Value
The Keysight Q347B Q-Band Noise Source is a valuable tool for engineers and technicians who need to test and characterize receivers and other RF components. It provides a reliable and accurate source of noise, making it an essential tool for any RF lab.
Additional information
| Brand | Keysight | 
|---|
 
			         
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                              
                             










 
                
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