SCD’s advanced 12μm VOx Microbolometer stands out as the ideal choice for VGA LWIR systems. With its exceptional image quality, remarkably low Noise Equivalent Temperature Difference (NETD), very low time thermal constant (Tau), rapid image acquisition, and minimal weight, SCD’s Microbolometer ranks among the leading LWIR sensors in the market. It is suitable for a wide range of applications, specifically tailored to meet challenges associated with Size, Weight, Power (SWaP) constraints and highly dynamic applications. This product continues SCD’s long heritage uncooled detectors technology, along with our 25μm and 17μm pitch families, fielded and combat proven for more than 20 years.

The ACTUS® ARKS5255 (5-25X, 56mm FFP) Long Range Riflescope is designed for precision and durability, meeting the needs of professional users across a wide range of environments. Equipped with a First Focal Plane (FFP) optical design, it enables fast and accurate target coverage at any magnification level. The illuminated reticle ensures smooth and clear targeting in low-light conditions, such as during dawn or dusk. Whether in challenging operational environments or critical moments, the ACTUS® ARKS5255 is the ideal riflescope for users seeking superior performance when it matters most.

The SDI170 IMU is designed for demanding, mission-critical, rugged environments and ideal for continuous use applications with no wear-out components, highly linear accelerometer performance and longer life compared to competing alternatives. It is constructed with EMCORE’s latest generation quartz gyros, quartz accelerometers, and high-speed signal processing to achieve outstanding precision performance. The solid-state quartz sensors and hermetically sealed IMU construction provide reliable MTBF and a 20-year operating and storage life. Continuous Built-in Test (BIT), configurable communications protocols, electromagnetic interference (EMI) protection and flexible input power compatibility make the SDI170 IMU easy to use in a wide range of higher-order integrated commercial and defense system applications.

A converter-integrated Main Generator installed in the T-50 series that supplies power to the system.

To complete their missions successfully in hostile territory, helicopters must have accurate, jam-resistant navigation systems that are able to operate effectively and dependably in all mission scenarios. These conditions may require high-speed, low-level flight over featureless, unknown terrain, and in the presence of enemy jamming.

This system product is a product that directly supplies and heats lubricant oil for smooth operation of the main engine cylinder’s metallic and mechanical movement. Lubricator, a product that supplies lubrication directly to the main engine cylinder liner, can control injection timing and consumption using an electronic control method that responds to the movement of the main engine piston. The alpha lubricator system is based on an algorithm controlling the cylinder oil dosage proportionally to the sulphur content in the fuel and, fuel consumption on particular load of engine. Minimum cylinder oil dosage is required to provide an adequate oil film and detergency properties. Everllence and WIN GD engines are currently applying the second generation Lubricator type, the Everllence type is Mk-I and the WIN GD type is Mk-ε (Epsilon).

공중 통신용 VHF/UHF 트랜시버 제품군 R&S®M3AR 제품군의 소프트웨어 정의, 다중 대역 지원 공중 트랜시버는 모듈식 설계와 첨단 기술로 높은 MTBF 값과 긴 수명을 제공합니다. 작고 가벼운 이 트랜시버는 뛰어난 성능으로 무인 항공기를 포함한 모든 유형의 항공기에서 작동할 수 있습니다. 언제든지 다른 파형을 설치해 사용할 수 있어 다양한 작전 시나리오에서 상호 호환이 가능합니다.

CATIS™ is an ultra-high-resolution, small satellite imaging radar device independently developed by Lumir. It consists of three components: the radar signal transmission/reception device SCEU, an active phased array antenna SATA, and a data downlink antenna KaPA. This X-band imaging radar device is designed for small satellites weighing 150 kg, offering an ultra-high resolution of 0.3 m. It transmits wideband RF signals to the observation area while orbiting at an altitude of 500 km and receives the reflected signals to acquire Earth observation data.