NEW INNO INSTRUMENT IFS-10 SALES and INNO INSTRUMENT IFS-10 CALIBRATION
 
Custom-Cal has for sale a new INNO INSTRUMENT IFS-10. Also, short calibration turn times minimize downtime and reasonable rates decrease your long-term cost of ownership and minimizes downtime of the INNO INSTRUMENT IFS-10. We specialize in quick turnaround times and we can handle expedited deliveries upon request.

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   INNO INSTRUMENT IFS-10   Description / Specification:    
INNO INSTRUMENT IFS-10 Fiber Master Core-Alignment Fusion Splicer

The INNO Instrument IFS-10 Fiber Master Core-Alignment Fusion Splicer with the New DACAS (Digital Analysis Core Alignment System) is one of the most dependable splicers on the market. The Fiber Master splicer features a rubberized design for field use in harsh weather conditions. The IFS-10 has a friendly, intuitive GUI (Graphical user Interface) with a 5 inch color LCD screen that is easy to see and is adjustable for front and rear splicer orientation. The sizeable, large battery capacity at full charge allows for up to 350 splices. Amazingly, the IFS-10 splicer is the most reliable and user friendly Core Alignment splicer in the world. Specifications. Splicing Method: Core alignment (DACAS:Digital Analysis Core Alignment System). Average Loss: SM(0.02dB) | MM(0.01dB) | DS(0.04dB) | NZDS(0.04dB). Return loss: >> 60 dB. Splice Time: 9s average SM | 7s SM Quick Mode. Pull Test: 1.96 ~ 2.25N (standard). Electrode Lifespan: > 2,500 arcs. Applicable Fiber: SM(ITU-TU.652), MM(ITU-TU.651), DS(ITU-T G.653),NZDS(ITU-T G.655), G657A, G657B. Cleaved Length Coating: diameter < 0.25mm = 8-16mm, Coating diameter > 0.25mm = 16mm minimum . Coating Diameter: 100 to 1000 um. Cladding Diameter: 80 to 150 um. Heating Programs Preset: 10 heating modes. Heating Time: FP-03 typical heating time 30 s. Protection Sleeve: 60mm, 40mm. Data Output: USB master device and COM. Splice Programs: 100 user mode. Splice Memory: Up to 2000 records. Battery: Typical full cycle 350 Splice and Heat. Power Supply: AC 100-240V input or DC 10-15V. Monitor: Color 5" LCD monitor, with tempered glass. Cameras ; 2 CCD camera system. Magnification: XY style: 150 power, X/Y: 300 power. Fiber Display: X/Y or XY, single X.Y. Weight: 2.2KG (without battery)


Additional Repair Services / Information.


Maintenance Available

 

Standard Calibration $475.00 *
*This is a Web introductory price for one calibration of the INNO INSTRUMENT IFS-10. 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.

Absolute Wavelength Accuracy
Absolute Wavelength Accuracy is the maximum difference between the actual wavelength and the displayed wavelength of the Optical Source. Wavelength is defined as wavelength in vacuum.

Decibel (dB)
A unit of measurement of optical power which indicates relative power. A -10 dB means a reduction in power by 10 times, -20 dB means another 10 times or 100 times overall, -30 means another 10 times or 1000 times overall and so on.

Nanometer (nm)
A unit of measure used to measure wavelength of light, meaning one one-billionth of a meter

Relative Intensity Noise (RIN)
Relative intensity noise (RIN), describes the instability in the power level of a laser. The noise term is important to describe lasers used in fiber-optic communication and LIDAR remote sensing. It is the square of the (spectrally resolved) RMS optical power amplitude divided by the measurement bandwidth and the square of the average optical power, expressed in dB/Hz.

Total Return loss
In an optical fiber, the loss that takes place at any discontinuity of refractive index, especially at an air-glass interface such as a fiber endface, at which a fraction of the optical signal is reflected back toward the source. RL = - 10log10 (Preflected/Preference)

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