The SWIR & NIR 25-250mm f/5.5 (NFOV) f/4.0 (WFOV) continuous zoom lens is a first to market low-Size, Weight, and Power (SWaP), compact lens, for the newly introduced 5μm SXGA, as well as for 10μm SXGA, and 15μm VGA SWIR detectors. The SWIR & NIR zoom lens employs a unique mechanical and optical design, resulting in an all-around smaller and lighter unit with only 860gr in weight, and 224mm in length, making it approximately 60% lighter than similar existing SWIR lenses. The SWIR lens is also chromatically corrected to support a broader short-wave IR wavelength regime from 0.7-1.7μm and operates with minimal distortion. The SWIR & NIR 25-250mm f/5.5 (NFOV) f/4.0 (WFOV) continuous zoom lens presents an unrivaled combination of SWaP capabilities, detection range exceeding 26km. Product features: • Continuous zoom in the 0.7-1.7μm SWIR regime • Designed for 5μm, 10μm SXGA & 15μm VGA SWIR detectors • Lightweight (<860 gr) • Detection range >26 km • Enables laser-line detection

JEFF FIREFLY is a perfect sunglasses for protecting the eyes and preventing reflection during daily or guard work. The glasses block wind and dust to protect the eyes. The Anti-Scratch & Anti-Fog coated polycarbonate lenses give you UV protection below 400nm. The TR-90 frame offers reliable comfort during use, as it is resistant to temperature changes even in extreme conditions such as deserts or harsh climates. Also, JEFF FIREFLY is comfortable to wear for a long time due to its lightweight fitting.

The 200W High Power Amplifier is an L-band amplifier that delivers 200W output with a 60% duty cycle. It provides a gain of over 53 dB, with output flatness of 2 dB depending on the input signal level. At maximum output, it offers ACLR performance of -20 dBc. With a built-in output-stage bandpass filter (BPF), it achieves excellent harmonic suppression of -70 dBc. Built-in monitoring functions include output signal and temperature monitoring.

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

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.

The main wheel assembly refers to the complete structural unit that includes the wheel, tire, axle, bearings, and in most cases, the braking system. As the primary load-bearing gear, the assembly is engineered to absorb high-impact forces during landing and provide strong braking performance during deceleration. Its design integrates durability, safety, and serviceability, making it a critical element of aircraft ground operations.

The L-band 8-channel filter bank receiver module is equipped with eight internal filter bank channels, enabling improved reception performance by isolating specific sub-bands within the receive frequency range. A 100W limiter at the input stage protects the receiver from high-power signals, and the module offers a low noise figure of 3.0 dB or less. The input P1dB for the receiver is -20 dBm, and the module features a built-in path self-test function.

Vulcanized Bonding - Complex Elastomer-to-Metal Bonding