Seedcore’s VPX Chassis Housing Assembly is designed as a structural platform for Multi-function radar signal processing systems. Featuring a robust 8U 2×5 slot VPX configuration, precision-machined aluminum construction, and excellent thermal management, it ensures high mechanical stability and optimal heat dissipation in demanding defense environments. This chassis housing is deployed in Korea’s key air defense radar systems, including the L-SAM, M-SAM, and LAMD programs, supporting mission-critical radar signal processing architectures.

The Ophir® SupIR 80-1200mm MWIR f/5.5 and SupIR 60-1200mm MWIR f/4 lenses are designed for 15 µm 640x512 and SXGA 10 µm pitch FPA (focal plan arrays) cooled MWIR detectors, respectively, providing detection ranges exceeding 28 km. Key Features: - High performance IR continuous zoom lens - Compatibility with 10 µm SXGA/HD and 15 µm 640x512 cameras - Maintains accurate LOS & focus through the full zoom range - Designed for extended range observation & C-UAS systems - Detection range exceeds 26 km

The Series 23 SuperNine® advanced performance MIL-DTL-38999 connector series provides many of the technology advances exceeding MIL-DTL-38999 Series III. Higher mating cycles, integrated banding porch, PC Tail and standoff availability and crimp termination Hermetics are all part of the family.

PTO SHAFT, Proven Performance, Realized in Reality CTLA's Power Transmission Shaft (PTO-shaft) is a key component of the aircraft secondary powertrain, transmitting the high-speed rotational power generated by the aircraft engine drive unit (EMAD) to the gearbox (AMAD). By applying high-strength, lightweight titanium material for the first time in the world, we have achieved both weight reduction and durability, while implementing outstanding stability and reliability through our proprietary electron beam welding technology optimized for high-speed rotation and high-speed precision balancing technology. In particular, this product, which is currently being mass-produced and delivered to the KF-21 fighter jet, has demonstrated excellent power transmission performance while minimizing vibration even in extreme environments. CTLA is leading technological innovation in the field of high-speed rotational machinery, spearheading the self-reliance of domestic aircraft components and advancing into the global market.

Key Features Enhanced speed and precision with a powerful 30W laser Supports a wide range of high-performance materials including Nylon 11, Nylon 12, and TPU Dimensions: 685 x 645 x 1065 mm Build Volume: 165 × 165 × 300 mm Weight: 114 kg (excluding build chamber or powder) Specifications 30W fiber laser Maximized powder reuse to minimize material waste ________________________________________

The ultra-low noise SRO-5680 GPS/GNSS-disciplined rubidium oscillator (GPSDO) features an EMI-shielded, rugged packaging, while integrating complex synchronization functionality all in one low-cost, super-small package. It is compatible with the FEI-5680 Rb model and utilizes the SmarTiming+® technology to provide a host of integrated GPS/GNSS disciplining and timing features. The SRO intelligently synchronizes, disciplines, and controls any primary 1PPS reference signal, such as GPS/GNSS, Cesium, Hydrogen Maser, and T1/E1, at cutting-edge 1ns resolution. Its slim and rugged packaging and ultra low noise features make it greatly suitable for next gen SATCOM, airborne and other stringent MIL applications. Applications: Mobile & wired telecom/datacom infrastructures Military communications, SATCOM & surveillance systems High precision instruments Time & frequency systems

Electric motor used to drive the joint (ST axis) of the Explosive Ordnance Disposal (EOD) Robot.

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.