The KX2-2046 is an X-band high-power MMIC amplifier fabricated on the GaN-on-SiC process. It operates from 8.0 – 10.5 GHz and typically provides 20W saturated output power with power-added efficiency of 46%. The KX2-2046 can support military and commercial radar systems. It is matched to 50Ω with integrated DC blocking capacitors on both RF input and output ports. The KX2-2046 is 100% DC and RF tested on-wafer. It is available in chip form. **Key Features** - Frequency Range: 8.0-11.5GHz - Small Signal Gain: 26dB - High Pout: 20W - High PAE: 46% - DC bias: Vd=28V @Idq=0.3A - Pulsed Vg: PW=100µs, DC=10% - Chip size: 2.95x1.66x0.1mm  

The radar that Raytheon Missiles & Defense is building for the U.S. Army has long been known as the Lower Tier Air and Missile Defense Sensor (LTAMDS). Now, ...

Large mirrors are crucial in various optical systems, particularly long-range multi-spectral setups for defense, surveillance, and commercial use, like UAV optics and agricultural temperature monitoring. Aerospace applications, such as satellites and telescopes, are common. These mirrors come in different shapes and materials, including Al, Si, Ge, and Cu, spanning visible, UV, and IR spectrums. By using advanced CNC grinding, polishing, and diamond turning we provide precise surface forms, with tight tolerances, and multispectral performance. Our mirrors, up to 700mm in diameter, provide impressive specifications: 0.05% radius tolerance, less than 0.5Fr P-V irregularities, 0.1Fr RMS at 0.633μ, and sub-40Å RMS roughness. MKS Ophir's proprietary coatings enhance spectral performance and surface durability. Contact us to set a meeting at ADEX Seoul

The SCFAN-CTRL-5U is an internal fan control module installed inside the chassis to manage cooling performance. It integrates with FAN trays and operates through Kontron’s Power Supply Control Module (PSCM) to control up to one 12V @ 3.5A fan and seven 12V @ 2.5A fans. This module ensures efficient thermal management and stable system operation in high-performance VPX-based embedded systems. It is deployed in the M-SAM-II multi-function radar system, providing reliable and optimized cooling control for mission-critical environments.

Whether satellites, spacecraft or space debris – GESTRA, the "German Experimental Surveillance and Tracking Radar", is a state-of-the-art radar system for observing and tracking objects in space. It operates in the microwave range and explores the Low Earth Orbit of 300 to 3,000 kilometres, i.e. the range in which most satellites and the International Space Station (ISS) are located. This makes it possible, for example, to protect space systems or the ISS from a collision with debris particles by providing a timely warning. Millions of tiny particles orbit the earth and, at a speed of around 28,000 km/h, pose a threat to active space technologies. GESTRA was developed and built by the Fraunhofer Institute for High Frequency Physics and Radar Techniques FHR on behalf of the German Space Agency at DLR.

1) Fabrication - possible Dismension : ~ D 1200 mm - Surface Errors PV < 79 nm RMS < 12 nm Roughness < 2 nm(Typical < 1nm) 2) Lightweight - lightweight Ratio : up to 82.5 % - Rib Thickness : ~ 2 mm - Face Sheet : ~ 7 mm - Lightweight Design & Fabrication

Dual Narrow Linewidth Amplifier - 3kW per channel

24-7 non-stop operating RADAR for ceaseless aerial surveillance and early trajectory detection. Design and Manufacture - Antenna Housing - Driving Unit