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Shortwave Power Amplifier
OM4001A
The OM Power model OM4001A is designed for all short wave amateur bands from 1.8 to 29.7 MHz (including WARC bands) and all modes. It is equipped with a two ceramic tetrodes FU-728F.
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Shortwave Power Amplifier
OM2501A (OM3501A)
The OM Power model OM2501A and OM3501A are designed for all short wave amateur bands from 1.8 to 29.7 MHz (including WARC bands) and all modes. OM2501A is equipped with a FU728F or GU84B ceramic tetrode and OM3501A is with GU78b ceramic tetrode.
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Shortwave Power Amplifier
OM4001HF
The OM Power model OM4001HF is designed for all short wave amateur bands from 1.8 to 29.7 MHz (including WARC bands) and all modes. It is equipped with a two ceramic tetrodes FU-728F.
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Short-Wave Infrared Camera
Goldeye G-032
The Goldeye G-032 SWIR camera supports Power over Ethernet (PoE) and data transmission with up to 100 m distance. Thanks to the integrated image optimization, the Goldeye is distinguished by an excellent image quality.The fanless model is optimized especially for industrial applications. It enables an easy system integration thanks to various mounting options, screw locks, extensive I/O control as well as many machine vision features.
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Short-wave Infrared Camera
Goldeye CL-008 Cool
The Goldeye CL-008 is one of the fastest QVGA resolution short wave infrared (SWIR) cameras with Camera Link interface. With frame rates up to 344 fps at full resolution, versatile application fields can be addressed and processes can be sped up strongly. To enable low-noise imaging in the spectral range from 900 nm to 1700 nm, the camera is equipped with a nitrogen filled cooling chamber. It enables the thermo-electric cooler (TEC) to operate the sensor at a temperature of 5o C and avoids condensation.
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Shortwave Infrared Camera Core
Tau® SWIR
FLIR Tau® SWIR provides outstanding short-wave infrared image quality and performance over a wide range of imaging and light level conditions. It is the ideal OEM SWIR imaging module for applications like hyperspectral instrumentation, silicon inspection, electro-optical payloads, art restoration, and portable imaging. The Tau SWIR camera incorporates the FLIR high resolution 640×512 ISC1202 Indium Gallium Arsenide (InGaAs) 15-micron pitch focal plane array (FPA) and includes several advanced camera controls features.
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Sensitive Short-wave IR Fluorometer & Absorption Spectrometer
NS3 NanoSpectralyzer
A customizable, modular NanoSpectralyzer: In addition to its core function as a sensitive short-wave IR fluorometer and absorption spectrometer, the NS3 can be configured with any of the following spectral capabilities: Visible emission, extended SWIR emission, UV absorption, visible absorption, extended SWIR absorption, Raman. Up to 5 excitation lasers (405 to 830 nm).
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Shortwave Plus 50 MHz Power Amplifier
OM2000A+
Thank you for purchasing this new model of the OM Power’s RF power amplifiers line for HF and 50 MHz amateur radio bands. You now own, the OM2000A+, an automatic unit with no knobs, no rotaryswitches on the front panel, just two small switches and one large touch display.Smart design, modern conception, high reliability is the result of OM Power’s development and many years of experience with overall solutions and special attention with the design of the protection circuits.This product is covered by two years of warranty on the amplifier itself and one year for the tube.We wish you will have many years of trouble-free use of this equipment, lots of fun and successful contacts in the world of amateur radio.
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Mercury Argon Calibration Source
HG-1
The compact, low-cost HG-1 Mercury Argon Calibration Source is a spectral wavelength calibration source for UV-VIS-Shortwave NIR spectrophotometric systems.
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Aion
The Aion is a powerful SWIR camera core with sensitive detection at shortwave infrared range. The high-performance sensor and low noise feature offers best solution for OEMs and integrators for their demanding applications.
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SWIR Cameras
Our SWIR or Short-Wave Infrared imaging covers the wavelength range from 900nm to 1700nm. A large number of applications that are difficult or impossible to perform using visible light are made possible, with great results, using short-wave infrared (SWIR) imaging thus enabling the user to "See Beyond the Visible". SWIR is similar to visible light in that photons are reflected or absorbed by an object, providing the strong contrast needed for higher resolution imaging– unlike thermal images, that rely on radiated photons. At NIT, we offer unique SWIR cameras and sensors, see below for more information on our products.
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Solar Energy, PV Monitoring
Apogee silicon-cell pyranometers feature a monocrystalline silicon-cell detector that has the same spectral response as a PV module. The sensors quantify shortwave radiation being harnessed as electricity.
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Small InGaAs Line-Scan Camera Module With Square Pixels
XSL SQ Series
The XSL square (SQ) series, based on an in-house developed linear detector, offer affordable short-wave infrared (SWIR) line-scan images. The XSL SQ camera modules are able to image line rates up to 40 kHz. The modules come with an industry-standard CameraLink, GigE Vision or QTE Samtec interface.
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Uncooled InGaAs Line-Scan Camera with Square Pixels
Lynx SQ Series
The Lynx square (SQ) series, based on an in-house developed linear InGaAs detector, offer affordable short-wave infrared (SWIR) line-scan imagers. The Lynx SQ cameras are able to image line rates up to 40 kHz for demanding machine vision applications. The cameras come with an industry-standard CameraLink or GigE Vision interface.
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InGaAs Line-Scan Camera with Rectangular Pixels
Manx R Series
Based on a brand new, in-house developed InGaAs linear detector, the Manx rectangular (R) is a high-performance short-wave infrared (SWIR) camera providing high speed and quality line-scan imaging. At unprecedented line rates of up to 256 kHz (or 128 kHz), the Manx rectangular (R) stands as the fastest line-scan InGaAs camera available in the world.
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InGaAs Line-Scan Camera with Square Pixels
Manx SQ Series
Based on a brand new, in-house developed InGaAs linear detector, the Manx square (SQ) is a high-performance short-wave infrared (SWIR) camera providing high speed and quality line-scan imaging. At unprecedented line rates of up to 256 kHz (or 128 kHz), the Manx square (SQ) stands as the fastest line-scan InGaAs camera available in the world.
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NanoFluorescence Microscope
NFM
The NFM is a specialized optical microscope system custom-designed for imaging individual single-walled carbon nanotubes (SWCNTs) through their intrinsic short-wave infrared fluorescence. It is ideal for SWCNT studies in physics, chemistry, biomedicine, and environmental research. The NFM is the new, more affordable replacement for our pioneering NM1 Fluorescence Microscope.
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Tunable, Pulsed IR SW & LW OPO IR Source
Firefly-IR
Firefly IR is available in short-wave and long-wave models, providing broad wavelength coverage from 1.4-8.5 µm. The compact and sealed design requires no manual alignment, and can be used in a variety of applications in the lab and in the field. Wavelength selection and scanning is automated and performed via web browser or using a TCP/IP command set. Pulsed operation and high repetition rate provide high peak power and rapid data acquisition.
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SWIR Line-Scan USB3 Cameras
NECTA S Series
NECTA S, the SWIR line-scan model in NECTA camera family, is capable of high-resolution acquisition in short-wave infrared bandwidth, ranging from 950 to 1700 nm. This new SWIR camera can reach up to 40kHz line rate with 14bit A/D converter: its high-speed USB3 interface, an advanced I/O, together with a compact and rugged aluminum case, make NECTA S suitable for most demanding machine vision applications.
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Remote Sensing & Proximal Sensing Systems
Portable or handheld spectrometers (field spectrometers) and hyperspectral cameras (imaging spectrometers) are the ideal tools for spectral data acquisitions and ground truthing of remote sensing imagery. SphereOptics offers you a wide range of spectrometers for the visible (VIS), near infrared (NIR), shortwave infrared (SWIR), and thermal infrared (TIR) wavelength regions. More details about our single point spectrometers for the VIS-NIR-SWIR can be found here, and for TIR here.
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Radiometer
CNR 4
The CNR 4 net radiometer consists of a pyranometer pair, one facing upward, the other facing downward, and a pyrgeometer pair in a similar con?guration. The pyranometer pair measures the short-wave radiation. And the pyrgeometer pair measures long-wave radiation. The upper long-wave detector of CNR 4 has a meniscus dome. This ensures that water droplets role off easily and improves the field of view to nearly 180, compared with a 150 for a flat window. All 4 sensors are integrated directly into the instrument body, instead of separate modules mounted onto the housing. But are each calibrated individually for optimal accuracy.
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RF Testing & Engineering Services
RF Testing & Engineering Services
Our team has world-class radio frequency experience in defense contracting, design, engineering, manufacturing, quality, research, and testing. The staff at 360°RF includes numerous design patent holders, a sitting member of the CEA's (Consumer Electronics Assoc.) Standards Committee, as well as columnists, editors, and authors for trade publications and reference books, including Radio Shack, Antennas, Selection, Installation, and Projects, TV, FM, CB, Cellular, Satellite, and Shortwave.
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Line Scan Camera
Linea SWIR
Teledyne DALSA’s short-wave infrared (SWIR) GigE line scan camera features a cutting-edge InGaAs sensor in a compact package for a wide variety of machine vision applications.This high speed, high resolution camera is the first product in DALSA’s SWIR family. Linea SWIR features a cutting-edge InGaAs sensor in a compact package that is suitable for a wide variety of applications. With exceptional responsivity and low noise, this camera allows customers to see their products like never before. Linea SWIR is available as a 1k resolution camera with highly responsive 12.5 µm pixels, or a 512 resolution camera with larger 25 µm pixels
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Power Line Meter
The Line EMI Meter measures electromagnetic interference in a single-phase AC power line. It plugs into a wall outlet (mains socket) and requires no battery. It immediately displays total line noise in millivolts (range 1999 mV, resolution 1 mV) in the frequency range 10 KHz 10 MHz (the frequency limits at which sensitivity is of the maximum sensitivity). A speaker plays the sound of the EMI, amplitude demodulated, in order to identify the EMI source (such as an AM or shortwave radio station vs. a motor vs. an electric arc).
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Pyrgeometers / Four-Component Radiometer
EKO's pyrgeometers and net radiometers are used for meteorological observations of atmospheric radiations (radiations from clouds, water vapor, CO2 etc.) and the net radiation exchange between the earth and the atmosphere. Net total irradiance (shortwave + longwave) is typically measured by 4 component net radiometers or single component pyradiometers which have a single detector covering the full range. Pyrgeometers measure the long wave down welling radiation by means of a single detector facing the atmosphere. The Net longwave and down welling radiation can be determined by calculation.
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Small, Uncooled InGaAs line-scan camera with rectangular pixels
Lynx R Series
The Lynx R series, based on an in-house developed linear InGaAs detector, is a high-performance short-wave infrared (SWIR) camera providing high speed and quality line-scan imaging.The Lynx R cameras are able to image line rates up to 40 kHz, for demanding spectroscopy applications.The camera comes with an industry standard CameraLink or GigE Vision interface.Benefits & Features• High speed line-scan imaging up to 40 kHz (10 kHz for the 2048)• High resolution 1024/2048 Rectangular pixels option (12.5μm x 250μm)• CameraLink or GigE Vision interfacing
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Small InGaAs line-scan camera module with rectangular pixels
XSL R Series
Your product description goes here.The XSL R series, based on an in-house developed detector, offer high-resolution short-wave infrared (SWIR) line-scan images.The XSL R camera modules are able to image line rates up to 40 kHz, for demanding spectroscopy applications.The module comes with an industry standard CameraLink or GigE Vision, or a 16 bit Digital Video interface.Benefits & Features• High speed line-scan imaging up to 40 kHz (10 kHz for the 2048)• High resolution 1024/2048 Rectangular pixels option (12.5μm x 250μm)• CameraLink, GigE Vision or 16 bit Digital Video interfacing
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UV Lamp Weathering Test Chamber
Sanwood Environmental Chambers Co ., Ltd.
Sanwood is a company with professional research and development, sales of Bench-top UV test chamber,Bench-top UV lamp aging test chamber,Bench-top UV weathering test chamber,Bench-top UV aging test chamber,Bench-top UV aging test chamber for 23 years. Ultraviolet light in the sun is a major contributor to the durability of most materials. We use UV lamps to simulate the short-wave ultraviolet portion of sunlight, which produces very little visible or infrared spectral energy. We can choose UV lamps of different wavelengths according to different test requirements, because each lamp has different energy and wavelength in total UV irradiation. Generally, UV lamps can be classified into two types: UVA and UVB.
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Near-Field Probes 100 kHz up to 50 MHz
LF1 set
The LF1 near-field probe set consists of 4 shielded near-field probes used during the development process for emission measurement of longwave, medium wave, and shortwave frequencies on electronic devices. The probe heads of the LF1 set are designed for incremental detection of sources of electromagnetic interference on assemblies. First, the electromagnetic interference of the assembly is detected by the LF-R 400 probe from up to 10 cm. Then probes with higher resolution like the LF-B 3, LF-U 5 and LF-U 2.5 are used to more precisely detect any source of interference. The probe heads are designed for taking measurements at single pins and larger components. Near-field probes are small and handy. They have a current attenuating sheath and, therefore, are electrically shielded. They can be connected to a spectrum analyzer or an oscilloscope with a 50 Ω input. The H-field probes do not have an internal terminating resistance of 50 Ω.
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Amplifiers
Becker Nachrichtentechnik GmbH
Becker Nachrichtentechnik GmbH offers a large portfolio of high performance broadband RF amplifiers. Optimized for linearity, high dynamic range and low noise, they cover all widely used radio standards like cellular, satellite radio, TETRA/BOS, GNSS, GPS, 802.11, including the new bands for LTE-U. They amplify wideband radio signals from shortwave over UHF, VHF up to 18 GHz in 50 Ohm technology (I-band, G-band, P-band, L-band, S-band, C-band and X-band). They are used as compact RF drivers, antenna pre-amplifiers or RF boosters in a variety of applications ranging from tunnel radio coverage extension, over airspace radio monitoring to in-ear monitoring and can also be offered as 1U 19” rack variants. Due to their advanced design, the power consumption is significant lower than typical industry alternatives, saving cost at customers with respect to cooling.