N9320B RF Spectrum Analyzer (BSA), 9 kHz to 3 GHz

N9320B RF Spectrum Analyzer (BSA), 9 kHz to 3 GHz

Share:


N9320B RF Spectrum Analyzer (BSA), 9 kHz to 3 GHz

Key Features & Specifications


Professional performance for spectrum analysis from 9 kHz to 3 GHz
• Minimum non-zero span sweep time: < 10 ms
• Resolving power RBW: 10 Hz to 1 MHz
• Sensitivity DANL: -130 dBm, -148 dBm with preamp on
• Overall amplitude accuracy: ±0.5 dB

Robust measurement features for characterizing your product easily
• Built-in power measurements: channel power, OBW, ACP, SEM and TOI
• Built-in power meter function with Keysight U2000 series power sensor support
• Optional tracking generator and preamplifier
• Optional AM/FM, ASK/FSK demodulation capability

Accessibility and ease-of-use at your finger tips
• Customized power-on or “preset” enabled setups
• Standard USB and LAN interface
• Multiple language graphic user interface
• Free remote control PC software

Description

Regardless of whether your application is electronics’ manufacture, bench repair, RF education or R&D projects, you need a spectrum analyzer that is equipped with the essential functionality, required performance at an affordable price. The N9320B is designed to be the right answer for you.

Enhanced power measurement and easy automated test programming features
• The accuracy of frequency selective power measurements when characterizing your products is very important. With a newly featured digital IF, the N9320B provides measurement accuracy and speed you need to accomplish tasks easily
• Power meter functionality is a standard feature built-in with Keysight U2000 series power sensor support for highly accurate RF and MW power measurements
• Direct access to perform one-button power measurement functions offer channel power, ACP, OBW, SEM and TOI measurements
• For automated test programming, the N9320B provides industry standard SCPI language support and connectivity choices with USB and LAN. SCPI code compatible with Keysight ESA-L Series enables easy migration from ESA-L to the N9320B