• The Pulsar 320E provides the ultimate in lighting control for strobe-only, high power applications. 
• 2 outputs for controlling 2 lights independently, each capable of 50A @ 100V DC.

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.

• This ultra high intensity line light series is built to handle the most extreme line scan lighting requirements. 
• Provides an intensity level of 2,100 klx (working distance of 75 mm). 
• Pre-engineered for expandability in 150 mm (6”) increments up to 2400 mm (94.5”). 
• Available in multiple wavelengths. 
• In the event of abnormally high ambient temperatures, the device automatically shuts down when the housing reaches 60°C and resumes operation at 56°C. 

Note: Requires third party power supplies – refer to spec sheet.

NoiseKen simulators to reproduce fast rise-up noises which are generated when switching ON / OFF electric current on the inductive load. 

Since the pulse includes broadband frequency and its rise-up time is fast at 3ns or less, it can make the noise coupling dense and effective to reproduce the malfunctions of electronics equipment under the test. 

It can realize performance evaluation of electronics equipment's upon reproduction of line noises which are intruded to the power supply lines or induced noises onto the telecommunication lines.

• For use with the SL256 Pattern Projecting Spot Lights 
• Five field-replaceable standard patterns available 
• 0.050mm line width photolithography 
• Reticles include spanner wrench 
• Please contact Ai for custom reticle patterns

Coaxial cable assembly suitable for fixed wiring inside and between equipment used in the microwave band up to 100GHz (continuous operating temperature range: -30 to +85°C). 

These cables have excellent formability (shape-retention capability) that make wiring work easy and exhibit superior loss characteristics compared to semi-rigid cables. Standard connectors are SMA (m) straight connectors, although other connectors can be used as required.

• The IC Inline Controller provides steady and optimal current to lights from a small package when larger, more versatile discrete controllers are not necessary. 
• The IC provides continuous-on and DC gating on/off control as well as 0-10 volt analog dimming. 
• All ICS models employ reverse input polarity protection. 
• A wash down version is provided with any light to which it is attached is also wash down. 
• 0 – 100% Intensity Control with optional DCS-MP, purchased separately, will provide manual intensity control via an external potentiometer.

• The LL167 Series provides a focused line of illumination in a passively cooled design. 
• Only available in White (for color illumination in a similar package refer to our LL137 Series). 
• Provides a high intensity level of 472kLux (working distance of 75mm). 
• Available in pre-engineered sizes from 6” (152mm) to 96” (2438mm) in 6″ increments. 
• A 3″ (75mm) length option is also available. 
• Available intensity control provides illuminance adjustability for every 6″ increment via a 0 – 10v input

• IRIG’s A and B and NASA 36 time code inputs 
• +3.3V or +5V signaling 
• 1PPS Sync input 
• External Event (Time Tag) input 
• Three programmable pulse rate outputs 
• Match Time output 
• Industrial Temperature Range option 
• Optional on-board GPS option 
• Optional HaveQuick input/output 
• Optional IRIG B time code output