• Outstanding stability
• Fast switching speed
• Ripple-free response over standard waveguide bands

The NC5000A Series AWGN noise sources feature outstanding stability, switching speed, and ripple-free response over standard waveguide bands. The high stability of the NC5000A Series allows these units to be used in place of cumbersome gas tube noise sources.

Ripple in the output of noise sources has a direct effect on measurement accuracy, so Noisecom has tailored the response of the NC5000A Series so that ripple is minimized throughout the specified frequency range.

EMC test equipment to evaluate the resistibility of electronic devices and components when energy charged on a human body or object is discharged to the electronic devices and components. NoiseKen brand ESD simulator is available to see malfunctions or function declines of electronic equipment for appropriate evaluations compliant with IEC 61000-4-2 Ed.2 Test Standard, ISO 10605 Ed.2 Test Standard & ISO 10605 Ed.3 Test Standard. 

The ESS-S3011A features a function which enables the user to pre-program test settings to minimize setup errors as well as having the unit be incorporated into a remote or autonomous testing setup. Another feature that sets apart NoiseKen ESD guns to that of competitors is the discharging gun separation design which helps achieve the lightweight. 

For conventional ESD guns, that have generators that are inseparable from the gun, you may experience having to replace the whole unit even only when certain parts of the unit are broken. However, with the NoiseKen’s separation design, replacement parts can be minimized to lower the running cost.

Safran’s SEEING™ 130 Wide includes a unique medium focal length catadioptric optics, limited by diffraction only and with ultra-low distortion, offering perfect imaging over 35 mm full-frame image format. It is fitted with a 10megapixel sensor. 

SEEING™ 130 Wide enables high Signal to Noise Ratio for multispectral (MS), hyperspectral (HS) and low light level imaging. SEEING™ 130 Wide includes a spectral filter with 23 bands covering Blue, Green, Red, Near InfraRed and Red Edge MS, for a broad spectral range between 475 and 900nm. SEEING™ 130 Wide has a large Field of View of 6.3° x 4.3° / 54 x 36 km2 from a 500km/310 miles orbit.

In addition to its a thermal design within a robust structure, SEEING™ 130 Wide has a low SWaP, saving launch and operational costs.

• Complete solution - battery test, simulation & solar array simulator software included
• Highest power density up to 37 kW in 4U rack height (9.25 kW/U)
• Fastest and cleanest power available (fastest transient response and low output ripple and noise)
• Universal 3-Phase AC Input accepts 180 VAC to 528 VAC
• Longest manufacturer-based reliability guarantee: 5-year warranty
• Parallel system power up to 1.2 MW
• Output voltage up to 2,000 V
• Bidirectional output current up to ±150 A, up to ±4,800 A in parallel
• True extended wide-range autoranging output
• Regenerative to 95%
• Color touch panel user interface
• Seamless transition between source and sink
• Built-in islanding detection

• Expandable frequency range from 18 to 325 GHz
• 2 to 3 times better accuracy
• Automatic Nitrogen purge eliminates helium equipment
• Primary calibration standard
• Radiometer reference source
• SATCOM earth station conformance verifications

The all new Linea HS™ delivers line rates up to an incredible 400 kHz at 32k resolution — over 13 Gpixels/sec via CLHS interface. With up to 128 TDI stages (plus an extra 64 in HDR mode) for unmatched sensitivity and incredibly low noise, Linea HS excels in the highest speed, lowest light applications.

• High power density / low ripple and noise 
• High programming resolution with Ethernet interface 
• Constant voltage and current mode 
• Remote sensing 
• Isolated analog control and monitoring (optional)

Reproduces transient voltage surge phenomena generated in a vehicle and evaluates the immune resistibility of DUT against the surge. The output waveforms are five as high-repeating pulse, giant pulse, field decay pulse, trapezoidal waveform + high-repeating pulse and high repeating pulse + giant pulse.