EXFO FLS-2200 CALIBRATION and EXFO FLS-2200 REPAIR
 
A calibration by Custom-Cal is performed by engineers with extensive OEM experience. We have the expertise and the necessary standards to perform the EXFO FLS-2200 Calibration, onsite calibration may be available. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

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   EXFO FLS-2200   Description / Specification:    
EXFO FLS-2200 Broadband SLED Source

The Exfo FLS-2200 Laser Source is a high-power, SLED-based FLS-2200 Broadband Source family covers all the bands needed for telecommunications applications. It provides a broader spectral range and more spectral density in a singlemode fiber than a white light source. The highly stable FLS-2200 is ideal for broadband applications, coarse wavelength-division multiplexing (CWDM) network testing, and passive optical networks (PON) component manufacturing and testing, as well as fiber-optic sensing and spectroscopy. Two Sources, One Box for CWDM testing, the dual-SLED option, covering the S, C and L bands, enables accurate characterization of fiber links and their passive components, with a very cost-effective test setup. Use the 1300 nm/1550 nm source for dual-window couplers and for PON components. Designed for Component Testing EXFO’s FLS-2200 offers enough power along the spectrum to measure high-level insertion loss. By combining the FLS-2200 with an optical spectrum analyzer (OSA), you can efficiently qualify your components during development or perform pass/fail testing during production. Depolarization as sources are naturally polarized, it is possible to take advantage of EXFO’s M9700 and IQS-9700 Passive Depolarizers, to bring the degree of polarization to less than 5%. This is especially useful when measuring the average insertion loss or counteracting the polarization dependency of an OSA. High Spectral Density Stability is essential to ensure that the test setup produces accurate measurements, time and again. The more stable the spectrum, the less often a reference trace has to be acquired. This translates into better productivity. After a reference trace is acquired with the OSA, it can be subtracted to all subsequent traces. With no device under test (DUT) in the system, the resulting traces, centered around the averaged value, present the typical spectral fluctuations of the source. Single SLED (FLS-2200-04 and FLS-2200-23), Dual SLED (FLS-2200-SCL). Center wavelength (nm): 1610 ± 15 (FLS-2200-04), 1310 ± 20; 1550 ± 20 (FLS-2200-23), 1485 ± 15; 1570 ± 10 (FLS-2200-SCL). 3 dB spectral width (nm): > = 50 (55 typ.) (FLS-2200-04). Output power (dBm): 5 (FLS-2200-04), >=8 (FLS-2200-23), >=3.5 (FLS-2200-SCL). Minimum spectral density (dBm/nm): -20 (1565-1640 nm) (FLS-2200-04), -28 (1260-1360,1510-1590) (FLS-2200-23), -29 (1460-1625) (FLS-2200-SCL). Peak spectral density (dBm/nm): -10 (FLS-2200-04 and FLS-2200-23), -23 (FLS-2200-SCL). Total power stability (dB): 15 min ± 0.01; 8 hours ± 0.01 (FLS-2200-04), ±0.015 (FLS-2200-23 and FLS-2200-SCL)). Spectral density stability (dB): 15 min ± 0.01; 8 hours ± 0.015. Ripple (dB): 0.3. Fiber type (µm) 9/125. Size (H x W x D) 117 mm x 222 mm x 333 mm (4 5/8 in x 8 ¾ in x 13 1/8 in). Weight b 2.7 kg (5.9 lb). Temperature: Operating 0 degC to 40 degC (32 degF to 104 degF); Storage -40 degC to 70 degC (–40 degF to 158 degF). Relative humidity 0 % to 80 % non-condensing



 

Standard Calibration $185.00 *
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*This is a Web introductory price for one calibration of the EXFO FLS-2200. Price does not in most cases include measurement performance data. Pricing does include NIST traceable calibration and issue of a calibration certificate and calibration label. Pricing may vary slightly due to volume and location of laboratory supporting calibration. Volume pricing may apply. On-site fees may apply depending on logistics, location and volume of work to be completed during the visit.


Related Optical Terms and Definitions. For a complete list go to our  Terms and Definitions Page.

Bandwidth
Bandwidth is the difference between the upper and lower frequencies in a contiguous set of frequencies within which a fiber optic component, link or network will operate.

Extinction Ratio (ER)
Extinction Ratio is the ratio of two optical power levels, of a digital signal generated by an optical source, (example a laser diode), where P1 is the optical power level generated when the light source is "on," and P0 is the power level generated when the light source is "off." The extinction ratio may be expressed as a fraction, in dB, or as a percentage.

Optical Signal-to-noise Ratio (OSNR)
Optical Signal-to-noise ratio is the ratio between the signal power and the noise power in a given bandwidth. Most commonly a reference bandwidth of 0.1 nm is used. This bandwidth is independent from the modulation format, the frequency and the receiver. For instance a OSNR of 20dB/0.1nm could be given, even the signal of 40 GBit DPSK would not fit in this bandwidth. OSNR is measured with a Optical Spectrum Analyzer. It is generally measured at the wavelength of interest.

Repeatability
Repeatability is the variation in a number of repeated measured quantities when measurement conditions are changed and restored. The value corresponds to half the spread between the minimum and maximum value measured.

Wavelength Repeatability
Wavelength Repeatability is the random uncertainty in reproducing a wavelength after detuning and re-setting the wavelength. The wavelength repeatability is ± half the span between the maximum and the minimum value of all actual values of these wavelengths. Example test condition: uninterrupted TLS output power, constant power level, temperature within operating temperature range, coherence control off, short time span. Note: NOTE The long-term wavelength repeatability can be obtained by taken the wavelength repeatability and wavelength stability into account.

Please contact us for your EXFO FLS-2200 CALIBRATION and/or EXFO FLS-2200 Broadband SLED Source REPAIR
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