The CZ600IP is a high-performance un-cooled LWIR thermal camera engineered to deliver professional-grade imaging and system integration. With a 640x480 resolution and 12μm pixel pitch sensor, it provides exceptional clarity and detail, even in low-contrast environments. Its motorized focus and zoom control ensure smooth and accurate long-range observations, making it ideal for applications that demand both precision and flexibility. The camera’s wide temperature measurement range further enhances its utility, supporting reliable operation in industrial process monitoring, facility security, and advanced research projects.
Equipped with modern networking features, the CZ600IP supports Gigabit Ethernet connectivity, H.265/H.264 compression, and OnVif Profile S compliance, ensuring seamless integration with existing surveillance and monitoring systems. It also offers multi-streaming capabilities and advanced security protocols, allowing safe and efficient deployment in critical infrastructure. By combining robust imaging technology with flexible system compatibility, the CZ600IP stands out as a versatile solution that adapts to evolving customer needs while maintaining high reliability and accuracy.

The Haigh-Farr family of rugged Blade antennas is available in frequencies ranging from UHF to upper C-band. Since 1972, our blade antennas have a demonstrated reliability of use in high-performance airborne applications. In addition, they are used extensively in ground-based vehicles such as race cars, trucks, tanks, and motorcycles, to name a few. 60XX & 61XX Series: Our 60XX & 61XX Series blade antennas have quasi-uniform null-free hemispherical gain patterns and may be provided in either straight or rounded blade configurations. 60XX and 61XX Series blade antennas are available in standard and high powered versions. With sufficient airflow, our standard blades handle an average power of 25 - 30W CW and our High Powered blades can handle an average power of 80W CW. These blade antennas share a common footprint with varying height. Multiband: Haigh-Farr Multiband blade antennas utilize identical materials and construction as our 60XX & 61XX series blade antennas with additional bandwidth. UHF: Haigh-Farr UHF blade antennas provide coverage down to 380 MHz and up to 470 MHz in two unique form factors. Our 6300-X series of blade antennas utilize identical materials and construction as our 60XX & 61XX series blade antennas in the larger blade structure required at UHF-band. Our P/N’s 16230-XXX and 16400-XXX are low profile, mechanically robust designs that can be custom tuned to meet discrete UHF frequencies, with an option to add thermal protection for high temperature environments.

High-power laser weapons targeting objects at 0.5 ~ 4.0km distances require optical components with sub-nm wavefront error precision. Our Company has successfully developed aspherical polishing and high-power laser coating technologies for Ø300 ~ 550mm optical components through defense project experiences. measurement technology 1) Laser Induced Damage Threshold(LIDT) - The evaluation to confirm the durability of optical components is called LIDT (Laser-Induced Damage Threshold), which is defined as "the maximum amount of laser radiation incident on an optical component when the expected probability of damage is zero" (ISO 21254). In other words, it represents the maximum intensity or power of laser that an optical component can withstand, making it a critical requirement in laser weapon systems. - Our company has established LIDT measurement technology and in-house facilities developed in accordance with ISO 21254 standards. When compared with LIDT test results from domestic and international companies during laser weapon system development, we have demonstrated measurement technology and accuracy that meets or exceeds industry standards. While overseas companies require more than one month for verification processes, our company can immediately provide reliable data through our LIDT system. 2) Cavity Ring Down Spectroscopy(CRDS) - When the reflectivity is 99.997%, this may not present significant issues in low-power laser applications. However, in high-power laser components, even the 0.05% of light that passes through the optical mirror can cause problems in vulnerable parts of the system, including rear optical instruments, bonded lenses, and control cables. Therefore, measurement and evaluation methods for high-reflectivity optical mirrors are extremely important. - Currently, the transmittance and reflectance of optical components are generally measured using spectrophotometers, but measuring reflectance levels of 99.5% or higher is not possible with this method. CRDS (Cavity Ring-Down Spectroscopy) technology is required to achieve measurement resolution beyond that of spectrophotometers, and our company has established this system to measure the reflectance of various optical components. This is a critically important technology for responding to high-power laser weapon system development requirements.

- System Construction - U-Caster-HT: Network video transmission device - KASSO® server: Connects Tx and Rx in a cloud environment, streams video to the receiving device, and manages connected devices (settings, transmission/reception connections, etc.). - Video receiving device: MonaLisa-Rx device (U-Caster-HR) or computer/smartphone - Receiving playback software: Web browser or WebRTC streaming playback program

EO/IR Payload System EOTS (Electro-Optical Tracking System) is an electronic optical image tracking device that identifies danger and emergency situations on the battlefield, monitors and tracks tragets, and calculates their coordinates, and is an essential equipment for drones that can be used in both military and private sectors. M1 and M2 were developed to use a common mount that connects to the drone by keeping the size of the gimbal assembly the same at 4 inches. M1 can be recognized at a maximum of 0.2km for humans during the day and at night, and M2, which operates in adverse conditions at night, can be recognized at up to 1.0km for tanks in the form of IR continuous zoom.

The Glenair next-generation STAR-PAN NG ecosystem incorporates a range of new capabilities in direct response to requests from JTACs, special operations forces, mission commanders, and other military specialists. Design innovations in STAR-PAN NG have resulted in higher current-carrying capabilities, greater versatility in power input support, and real-time plug-and-play USB device integration. The STAR-PAN NG hub and cable series offers a number of interface improvements and circuit board innovation.

The maximum transmission distance varies based on the following frequency-related specifications. Camera Frequency Max Cable Length ================ =============== 20 ~ 60 MHz 10 m 60 ~ 80 MHz 7 m 80 ~ 85 MHz 5 m The PoCL Bypass function supports Power over Camera Link (PoCL) operation from the Frame Grabber to the selected camera. However, the power supply to unselected cameras is automatically disabled. To prevent power cutoff, separate power must be provided to the cameras. Configurations are available as follows, including image signal amplification. [Features of CLM-30C4]  Fully supports the Camera Link interface (Area/Line Scan).  Provides manual (switch) or remote (RS232) camera selection.  Allows selection from one of four cameras configured for Base (Layer 1) or Medium/Full (Layer 2) levels.  Supports Base/Medium/Full setups (CC1~4, RS232, LVAL, DVAL, FVAL)  PoCL bypass function: Automatically powers only the selected camera when PoCL-compatible cameras, frame grabbers, and cables are used.  Supports pixel frequency from 20 to 85 MHz.  Supports PoCL signal bypass (patented).  Enables lossless transmission.  Provides additional full-duplex RS232 communication at up to 256 Kbps.  Features a locking DC power jack (Molex).

The AI Inspection Rover is capable of autonomous driving indoors and outdoors, obstacle avoidance, high-resolution image acquisition, aircraft underbody inspection, and platooning. Its low-height design allows it to pass under the aircraft, and with its zero-turn function, it can execute missions more efficiently. Additionally, it can drive slopes of up to 10° and overcome bumps of up to 30mm.