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 $550.00 *
*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.

Chromatic Dispersion
Chromatic Dispersion is a broadening of the input signal as it travels down the length of the fiber. Chromatic Dispersion results from a variation in propagation delay with wavelength, and is affected by fiber materials and dimensions.

Detector
A Detector is a signal conversion device that converts power from one form to another, such as from optical power to electrical power

Jitter
Jitter in technical terms is the deviation in or displacement of some aspect of the pulses in a high-frequency digital signal. Jitter is the time variation of a periodic signal in electronics and telecommunications, often in relation to a reference clock source. Jitter may be observed in characteristics such as the frequency of successive pulses, the signal amplitude, or phase of periodic signals. Jitter is a significant, and usually undesired, factor in the design of almost all communications links (e.g., USB, PCI-e, SATA, OC-48). In clock recovery applications it is called timing jitter.

Polarization Mode Dispersion (PMD)
Polarization mode dispersion (PMD) is a form of modal dispersion where two different polarizations of light in a waveguide, which normally travel at the same speed, travel at different speeds due to random imperfections and asymmetries, causing random spreading of optical pulses. It is he difference between the maximum and minimum values of loss typically measured in ps/km^1/2.


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