Bristol Instruments- 828 Series Optical Wavelength Meter

The fastest wavelength measurement for optical transceiver testing

The 828 Series Optical Wavelength Meter from Bristol Instruments is designed to revolutionize the production of tunable transmitter lasers used in WDM applications.

A Fizeau etalon design is used to generate a spatial interferogram that is detected by a fast InGaAs photodetector array. An on-board digital signal processor quickly converts the interferometric data to wavelength. Because this calculation is done within the instrument, a sustained measurement rate of 1 kHz is achieved.

This speed enables greater efficiency in the production of WDM transceivers by dramatically reducing the time needed for wavelength testing.

 

Accurate wavelength measurement is guaranteed

Two versions of the 828 Optical Wavelength Meter are available. The model 828A is the most precise, providing an accuracy of ± 0.3 pm. For less exacting test requirements, the 828B system is a lower-priced alternative with a wavelength accuracy of ± 1.0 pm.

Automatic calibration with a built-in wavelength standard maintains the performance of the 828 Optical Wavelength Meter over long periods of time. What’s more, every 828 system is rigorously tested with laser sources that are traceable to NIST standards.

 

Designed for convenience, built to last

Operation of the 828 Optical Wavelength Meter is straightforward.

The optical signal enters the model 828 through an FC (UPC or APC) fiber-optic connector on the front panel. The system’s high sensitivity results in an input power requirement as low as -40 dBm (0.1 µW). Automatic attenuation instantly adjusts the signal for optimum performance.

A convenient touch-screen display on the instrument’s front panel controls the 828 system and reports the measured wavelength and power. The measurement data can also be sent to a PC using a variety of interface options that satisfy virtually any test application.

An RS-422 serial interface is available for data streaming that can be triggered by the instrument itself or with a user-supplied signal. As many as one million measurements can be stored to an internal data buffer for analysis at a later time. Or, interfacing can be done via a library of SCPI commands using a standard USB or Ethernet interface, or an optional GPIB interface.

The rugged design of the 828 Optical Wavelength Meter provides long-term reliable operation that is backed by a five-year warranty covering all parts and labor.

Halogen & Deuterium Halogen light sources

Avantes Deuterium light sources are known for their stable output ad are used for UV absorption or reflection measurements. These can also be used as irradiance calibration sources due to their high stability. The standard AvaLight-DH-S mixes the halogen light with the Deuterium light, thus producing a wide spectral range light source. The output spectrum of Deuterium light sources exhibits several peaks, with a prominent peak at 656 nm. The AvaLight-DH-S-BAL incorporates a dichroic beam splitter installed to minimize these peaks, providing a smooth spectrum from 200-2500 nm.

Xenon light sources

Our pulsed Xenon light source is used in applications where a long lifetime and high output power is needed, such as in fluorescence measurements. This is an affordable UV source, but the spectral output is not as smooth and continuous as the AvaLight Halogen and Deuterium light sources.

LED light sources

LED light sources provide high power at a precise wavelength. A typical application for AvaLight-LED sources is fluorescence. They provide a long lifetime, short warm-up time, and high stability.

Calibration light sources

For wavelength calibration, Avantes offers a variety of sources including Argon, Mercury-Argon, Neon, Zinc, and Cadmium. All Avantes spectrometers are factory wavelength calibrated and do not require recalibration as they have fixed slits and optics. For those customers who wish to do their own calibrations, the AvaLight-CAL light sources can be used for recalibration purposes. For auto-calibration, AvaSoft-Fill provides a calibration procedure to make this easy.

OCAM² EMCCD Cameras

OCAM2K and OCAM2S are high speed low noise EMCCD cameras able to run at 2067 fps (3700 fps in binning) with subelectron readout noise.

C-BLUE One

C-BLUE One is an ultra-high performance scientific CMOS camera specifically designed for demanding imaging applications in the visible range (400 nm – 1000 nm).

C-BLUE One UV

C-BLUE One UV is an ultra-high performance scientific CMOS camera specifically designed for demanding imaging applications in the UV and visible range (200 nm – 1000 nm).

C-RED One

C-RED One is a ultra high-speed photon counting SWIR camera using a unique 320 x 256 pixels HgCdTe e-APD array with 24 μm pixel pitch.

C-RED 2

C-RED 2 is a revolutionary high speed low noise SWIR camera able to run at 600 fps with a very low noise under 30 electrons and ultra low dark under 600 e/p/s.