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.

IP66-rated waterproof and dustproof design Intel® Alder Lake Core™ i3-N305 with 8 E-cores -40°C to 70°C temperature operation 2x 2.5GbE via M12 X-coded connectors 1x isolated RS-232, 1x isolated RS-422/485 via M12 A-coded connectors 3x isolated DIO and 1x CAN2.0B via M12 A-coded connectors Low power and high endurance FRAM for data logger Class 1, Division 2 and ATEX certification in hazardous area applications 8V to 35V DC input with ignition power control input via M12 A-coded connector

STERNA System accurately finds True North in virtually all terrains and regardless of the weather conditions. The performance of STERNA System is not disturbed by gear carried by its operator or if used next to heavy armored vehicles. It remains highly accurate even when deployed on reinforced concrete floors or in dense urban settings. STERNA System operates reliably even in GPS denied environments and does not require the operator to carry any support resources to determine True North. If your mission success depends on the highest level of accuracy and precision, there is no substitute for STERNA System.

The Ku-band Amplifier Module is a low-power amplifier designed to amplify the LO (Local Oscillator) frequency in the Ku-band. It provides a gain of at least 17 dB and an output level of 13 dBm or higher. The module includes a built-in monitoring function for output signal detection.

Titanium Grade 1 -Strip Titanium Grade 2 -Bars-Sheets and Plates-Tubes and Pipes Titanium Grade 4 -Bars-Sheets and Plates-Wire Titanium Grade 5 (6Al-4V) -Bars-Sheets and Plates Titanium Grade 5 ELI -Bars-Sheets and Plates Titanium Grade 7 -Bars-Sheets and Plates-Tubes and Pipes Titanium Grade 9 (3AL2.5V) -Tubes and Pipes Titanium Ti-6Al-7Nb -Bars

The French aerospace sector is a leader in Europe and in the world. GIFAS protects this number-one status that enables our country and its industry to assert itself on the international stage. The development of our industry has been possible thanks to a constant dialogue with our international partners.

ts advanced integrated optics and closed-loop Field Programmable Gate Array (FPGA) electronics deliver much higher accuracy, lower noise and greater efficiency than competing technologies. In addition, the EG-1300 can be calibrated internally for better thermal effect and has both digital and analog outputs, along with separation of the electronics from the FOG’s sensing coil assembly to accommodate the widest variety of installation parameters. Features Fully-integrated optics and electronics Advanced optics and FPGA electronics for higher accuracy, lower noise and greater efficiency Precise navigation (1 mile/hour without GPS) Fast, precise gyrocompassing to 1 milliradian Bandwidth to 500 Hz Separate electronics and sensor modules More economical than competing systems Applications Navigational grade applications Unmanned aerial vehicle (UAV) guidance Missile guidance Aeronautics and aviation Robotics

Input : 24VDC Output : 270VDC N+1 System