TESCAN SOLARIS is a fully automated sample prep platform optimized for advanced devices with sub-10 nm features. It integrates the Triglav™ SEM, AutoTEM Pro™ software, and OptiLift™ nanomanipulator to enable hands-free, repeatable lamella prep in planar, inverted, or top-down geometries.

Key Features Revolutionary speed enabled by advanced LFD technology High-resolution and highly accurate prints Compatible with a wide range of resins including functional and engineering materials Dimensions: 390 × 367 × 554 mm Build Volume: 200 × 125 × 210 mm Weight: 18.3 kg Specifications XY Resolution: 25μm Minimum Layer Thickness: 25μm Maximum Print Speed: 100 mm/hr

Depending on the applications of our customers we offer a very wide range of technical solutions of assemblies and / or mechanical subassemblies with various characteristics. ABC offers a wide range of solutions ranging from micro-mechanics to large systems, based on standard solutions already developed and / or customized solutions as needed by the customer.

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 most advanced flightline test set available, capable of testing all Alternate Mission Equipment (AME) and Aircraft Armament Equipment (AAE) including pylons, launchers, bomb racks, and pods. Overcoming the legacy and "smart" weapons armament test gap, SmartCan utilizes active test and weapons emulation for all currently deployed weapons systems' communications interfaces.

정상적인 신호 수신을 방해하는 재밍 (Jamming)을 극복하고 안정적인 위성신호를 수신하는 안테나를 독자개발하였습니다.

[LEO GNSS-R] Satellite : LEO RF Characteristics : GPS L1/L5, Galileo E1/E5a(option) Accuracy : Position ≤ 10m(3DRMS), Velocity : ≤ 1m/s Raw Data Accuracy : Pseudo-Range : 1m(RMS) Carrier-Phase : 10mm(RMS) Data Output Rate : 1Hz 1PPS Accuracy : Sync to GPS Time Data < 1us (1PPS Accuracy < 1.5us) TTFF : Cold Start ≤ 20min / Warm Start ≤ 10min Dara Interface : MIL-STD-1553B, RS-422(Data Interface) [GEO GNSS-R] Satellite : GEO RF Characteristics : GPS L1/L2C/L5, Galileo E1 Accuracy : Position :: ≤ 30m(3DRMS), Velocity : ≤ 1m/s Raw Data Accuracy : Pseudo-Range : 1m(RMS) Carrier-Phase : 10mm(RMS) Data Output Rate : 1Hz 1PPS Accuracy : 2us(RMS)/Sync to GPS Time Data TTFF : Cold Start ≤ 45min / Warm Start ≤ 20min Dara Interface : MIL-STD-1553B EEE Parts : ITAR Free Parts

Plane Windows are used as substrates for a variety of applications, such as laser window, output couplers, beamsplitters, beam combiners, mirrors, dichroic filters and plate polarizers. Considerations in selecting window substrates include transmission range, absorption coefficient, incident laser power density and environmental factors such as pressure, temperature, moisture, abrasion and corrosion. Plane Windows listed under UV / VIS / NIR substrates are specified for applications involving coating wavelengths 193nm ≤ λ〈2.0 μm. Units for these substrates are given in mm. Plane Windows listed under IR substrates are specified for applications involving coating wavelengths λ≥ 2.0 μm. Units for these substrates are given in inches. Refer to the THIN FILM COATINGS section for information on coatings that can be applied to these substrates.