• Output White Gaussian noise
• 127 dB of attenuation; 0.1 dB step size
• Units > 2 GHz have total attenuation of 79.9 dB
• Low distortion signal path
• Noise attenuator accuracy:
  • ±0.2 dB or 0.5% at 1 – 500 MHz
  • ±0.2 dB or 1% at 0.5 – 1.0 GHz
  • ±0.3 dB or 2% at 1 – 2 GHz
• Standard connectors SMA female
• Power 115 VAC, 60 Hz; 110 VAC, 220 VAC
• Operating Temperature: -10° to +65°C

Not all amplifiers are created equal, so how can you be certain that an amplifier will work for your needs? You deserve to be confident that the amplifiers used with your test-and measurement lab benches will meet the requirements of your specific applications, are reliable, and are equally well-supported pre-and post-sale. When it comes to application expertise, reliability and support, there is no company that does it better than Maury.

• Ideal for applications requiring high ENR and immunity to large incident RF power
• Low VSWR
• Built-in isolator

The NC3400 Series coaxial AWGN noise sources are an excellent choice for applications requiring high ENR and immunity to large incident RF power, such as ATE, radiometer, and radar systems. The calibration accuracy and flatness of the NC3400 Series noise sources are enhanced by their low VSWR. The built-in isolator provides almost constant output impedance as the noise source bias is switched on and off. The isolator also protects the noise diode from incident RF power (consult the factory for higherpower units).

An SMA female connector is standard for the RF output and a BNC female connector is standard for the bias input. Other connectors are available as options.

• Single system power up to 650 kW Parallel system power up to 1.3 MW 
• Output voltage up to 1,000 V 
• Bidirectional output current up to ±1,000 A, up to ±2,000A in parallel 
• Available in 1, 2 or 4 channel configurations 
• Multiple channel units share internal DC Bus up to 2MW without drawing additional power from the AC Grid 
• Regenerative to 96% 
• Large 15-inch color touch panel 
• Short circuit proof 
• Designed for safety to EN ISO 13849-1 
• Dedicated Battery Testing/Simulation Modes 
• Seamless transition between source and sink 
• High reliability, long life components

• SPA available from 70KHz to 20/40/70/110/125/145 and 220GHz. Also available for banded configuration to 1.1THz.
• Dual SPA mode available: suitable for Mixers/Amplifier/ Harmonics /Spurious testing.
• SPA available on all ports. User can define which port to use as SPA port.
• Several detection types available in classical mode: Peak, minimum, RMS, Mean.
• Various math functions can be applied on SPA mode like Min hold/max hold/ user defined equations.
• Sources and receivers can be independently configured. Can be used as Tracking Generator.
• For units that have a dual source, a dual drive option is available. Support for external source control also possible.
• Phase synchronization for units with Dual source available. This feature allows users to control and configure the phase between the two sources.
• Source and receiver attenuator available with VNA can be activated in SPA mode. Recommendation to use option 62 (with attenuator on receiver side) for measuring the spectrum content of high-power devices.
• Software option: easy to install and upgrade existing user equipment.

The VULP 9118 E is a polarized log-periodic antenna

• (50) 75 - 1500 MHz
• 1 kW (w/ 7-16 High power 5.4 kW)
• Type N (female) or 7-16 DIN (f)

Bus simulator includes BPMU and SPU 

• Provides enhanced measurement and data-logging of up to 40 channels. 
• Bus Power Monitoring Unit (BPMU) can be easily relocated to TVAC chamber to ease cabling complications 
• Data can be viewed either in spreadsheet or graphical format 
• Spacecraft (Payload) Protection Unit (SPU) provides 10 μsec reaction to out-of-tolerance conditions