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C-band

1) IEEE designated frequency range from 4 - 8 GHz and a wavelength 7.5- 3.75 cm. 2) IR optical comms wavelength range 1530-1565 nm.

See Also: Band, Ka Band, E-band, Ku band, L Band


Showing results: 16 - 30 of 89 items found.

  • Amplified Spontaneous Emissions (ASE) Sources

    Apex Technologies

    The AP505xA series, high power ASE sources provide stable output power up to + 23dBm and broad flat spectrum over C+L band or T band. They enable effective and efficient measurements for component characterization or optical sensing. Finally, these products are proposed in friendly-user stand alone benchtop instrument with touch sensitive screen, GPIB, ethernet, RS-232 or USB controls.

  • Pulse Generators

    Schwarzbeck Mess Elektronik

    Calibration-Pulse Generatoracc. CISPR 16for Band A, B, C, D(9 kHz-1000 MHz)To calibrate the pulseresponse of EMI receivers.Pulse repetition frequency main generator 0.1 - 200 Hz (aux. generator up to 1 MHz) with IEEE-488 Interface.

  • Dual L/S Band SSPA

    Teledyne Paradise Datacom

    ​​Both S- and L-band frequencies have been the industry’s bands of choice for positioning and tracking applications like global positioning systems (GPS) and Tracking, Telemetry, and Control (TT&C) for satcom. This new dual S/L band SSPA offers customers a virtual ”two for the price of one” solution that dramatically lowers the costs of command and control, leaves a much smaller footprint, but also delivers higher reliability compared to traditional klystron power amplifiers.

  • Full C-Band or L-Band Tunable Laser Source

    LTS-2000 - Hangzhou Huatai Optic Tech. Co., Ltd.

    The LTS-2000 series full C-Band or L-Band quick adjustable laser optical source , is a 2U small model of high precision and muti-function, can be set up 1~4 port independent C or L band adjustable optical source. Various flexible configurations optional (see more in product series) , and makeing daily test and measurement applications greatly convenient.

  • Multi-band, High Precision GNSS Antennas

    ANN-MB series - u-blox AG

    Multi‑band (L1, L2/L5) active GNSS antennas with excellent price performance ratio. Supports GPS, GLONASS, Galileo, and BeiDou. Fast and easy antenna solution for high precision applications. Versatile mounting and connector options. Extended temperature range: up to +105 ° C.

  • Tunable Laser Source - MATRIQ

    Quantifi Photonics Inc.

    The Laser 1000 Series is a fully-compliant micro-ITLA laser with up to four channels in a compact benchtop form factor.Offering 0.01 pm resolution tunability across C or L bands, exceptional power accuracy up to 16.5dBm, and optional dither suppression, this is a versatile and cost-effective general purpose instrument.

  • Waveguide Gunn Oscillators

    Pasternack Enterprises, Inc.

    2 Models with Popular K and Ka Band Center frequencies of 24.125 GHz and 35 GHz. Designs feature mechanical tuning capabilty ranging up to + 3 GHz. Excellent Phase Noise Performance as low as -98 dBc/Hz typical. +10 dBm Output Power with Frequency Stability as low as -0.2 MHz/°C. Models have an Operational Temperature Range of -40°C to +85°C. Compact Aluminum Packages have Precision Machined Cavities that exhibit Optimum Performance. Fully Integrated Mil Grade WR-28 and WR-42 Waveguide Ports.

  • Airborne Receivers & Bit Synchronizers

    Lumistar Inc.

    The Lumistar LS-28-DRSM Series Multi-Mode Multi-Band Receiver/Combiner/TM Processing Unit is designed using ruggedized packaging to survive severe airborne conditions. The LS-28-DRSM is available in several configurations: 1) Airborne receiver only (RF to bits), 2) Airborne bit synchronizer only, 3) RF to TM Processing and Display (RF to bits to UDP decom to LAN Client Displays). Models with receivers are available in any band form 200 MHz to 7 GHz with S, lower L and C bands as standards. Other RF bands are available, please consult the factory for details. This unit can be mated with other Lumistar products to provide a complete air-to-ground re-transmission system.

  • Blackbody System

    IR-563/301 - Infrared Systems Development Corp.

    IR-563 is a ideal source for the Near (1-3 um), Mid (3-8) and Far (8-30+ um) infrared bands. The IR-563 has been the industry standard 1000º C blackbody for more than 30 years, and continues to provide excellent service to infrared applications throughout the industry. The IR-564 extends the temperature range of the IR-563 to 1200º C by changing cavity materials to Silicon Carbide and high purity Alumina ceramics, otherwise the two units are virtually identical.

  • Scientific SWIR Camera

    1280SCICAM - Princeton Infrared Technologies, Inc.

    This non-ITAR reduced weight (3000g) lattice matched, InGaAs scientific SWIR camera allows for high resolution SWIR imaging at 1280x1024 with high frame rates >93 frames per second (fps) at full frame size. This small pitch array,12 μm, combined with the high quantum efficiency of lattice matched InGaAs enables impressive imaging in the SWIR and visible spectral bands. The SWIR camera has the capability of four temperature setpoints, -20°C (no cooling), 0°C (fan cooling), -40°C, or -60°C (water cooled), using a 4 stage TEC integrated in a vacuum-sealed package. This advance digital array (PIRT1280A1-12) on board is a product of Princeton Infrared's decades of experience in InGaAs processing.

  • Lasers

    Alnair Laboratories Corporation

    A narrow-linewidth wavelength tunable laser source for applications such as coherent communication and long-range optical sensing. The laser can be locked to ITU grid wavelengths and fine-tunable with 1 MHz resolution. The laser can be controlled on the front panel or remotely via USB/GPIB. Benchtop version can host up to 4 separate lasers, with a combination of C- or L- band tunable laser.

  • K-Band Waveguide Gunn Oscillator Module

    FMWGN1001 - Fairview Microwave Inc.

    FMWGN1001 is a K Band Waveguide Gunn Oscillator with a Center Frequency of 24.125 GHz and a Tuning Range of +/- 1.0 GHz. The unit has a Phase Noise @ 100kHz Offset of -95 dBc/Hz typ and Frequency Stability of -0.4 MHz/°C max. The Gun Oscillator has an Output Power of 10 dBm min and Power Stability of -0.04 dB/°C max. The Waveguide Gun Oscillator uses a Bias Voltage of 5.0 Volts and a Bias Current of 200 mA and has a Waveguide Size of WR-42 with a UG-595/U Flange.

  • Point Contact Diodes

    Naprotek, LLC.

    SemiGen’s 1N Series of Point Contact Mixer Diodes are designed for applications through KA band. Each device in this series is specially designed for low noise gure, impedance and VSWR. Our devices are drop in replacements for all military and commercial requirements. These diodes employ epitaxial silicon grown in a speci c reactor for optimized performance. They are suitable for use in stripline applications.

  • Module Type Amplifiers

    FiberLabs Inc.

    Optical amplifier Gain Blocks are compact in size and suitable for built-in use. FiberLabs provides a wide wavelength range of optical amplifier Gain-Blocks over the O-, S-, C- and L-bands. These Gain Blocks can be used for B-PON system using three wavelengths of 1.31 μm, 1.49 μm, and 1.55 μm (ITU-T [compliant with G.983.3]), DWDM system and 100 GbE (IEEE 802.3ba) using the 1.3 μm band.

  • Optical Spectrum Analyzer Module Specification

    CA92001B - UC Instruments, Corp.

    UCINSTRUMENTS CA92001B C band optical spectrum analyzer module is a spectral engine for Process Analytical Technology applications. The OSA module acts as a stand-alone spectral engine, imaging and measuring a wide range of vapors, liquids and solids through transmission and diffuse reflection in a rapid non-destructive process. Leveraging our proprietary Micro-Optic technology, UC INSTRUMENTS’ C band OSA module features the following characteristics: (1) compact; (2) light-weight; (3) low power consumption; and (4) wide wavelength coverage. These characteristics of UC INSTRUMENTS’ compact OSA engines are suitable for a variety of handheld, portable or bench-top OSA/spectrometer applications. Equipped with a state-of-the-art internal wavelength reference, the OSA module is capable of precisely measuring optical spectrum. Because it does not require an expensive InGaAs detector array, the compact OSA module is a cost-effective alternative to other grating-based OSA/spectrometer engines. The OSA communicates with a PC or an instrument motherboard via an USB interface. UCINSTRUMENTS’ OSA module platform can be installed or co-packaged into existing NIR OSA/spectrometers as a cost-efficient alternative to other scanning optical engines.

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