AQ2200-232 Optical Sensor Head (Large diameter detector, 800 to 1700 nm), AQ2200-242 Optical Sensor Head (Large diameter detector, 400 to 1100 nm), AQ2200-202 Interface Module (2-channels)

AQ2200-232 Optical Sensor Head (Large diameter detector, 800 to 1700 nm); AQ2200-242 Optical Sensor Head (Large diameter detector, 400 to 1100 nm); AQ2200-202 Interface Module (2-channels)

  • Large-diameter detector for free-space measurement
    5 mm dia. (AQ2200-232), □5.8 mm (AQ2200-242)
  • Multi-core connector and cable measurement
    The AQ9340, AQ9436C and AQ9440C are required.
  • Power range: -90 to +15 dBm (AQ2200-232)
    -90 to +10 dBm (AQ2200-242)
  • Uncertainty: ±1.8% (1310 nm, AQ2200-232)
    ±2.5% (850 nm, AQ2200-242)
  • Averaging time: 100 µm (minimum sampling intervals)
  • Two sensor heads can be connected to the AQ2200-202 Interface module

What is an optical sensor type?

Optical sensors convert light rays into electronic signals to measure the amount of light and, in some cases, translate that information for an integrated measuring device to read. Optical sensors can measure either LED or laser light sources in a range of applications.

These are the types of optical sensors:

  • Point Sensors and Distributed Sensors
  • Extrinsic Sensors and Intrinsic Sensors
  • Through-Beam Sensors, Retro-Reflective Sensors, and Diffuse Reflection Sensors

 

I/L curve measurement of LD module
The I-L curve, drive current – optical power characteristics, of laser diodes can be measured accurately, quickly and seamlessly.
Because, the single-range power range of the new sensor head is as wide as 30 dB.
It enables to measure signals close to a threshold value at high resolution without changing the gain of amplifier circuit which takes extra time.

Experiment of free space optics
In experiments of free-space optics, optical parts are set on an optical bench or a breadboard, and the adjustment of optical alignment is most time consuming work.
The new optical sensor head is compatible with the 60 mm cage system.
It make it easy to build a optical experiment systems by combining with various cage system parts in the marketplace.

LCA 

Reduced emission of CO2 about 39% compared to the previous model.(AQ2200-232)
Results of Life Cycle Assessment.

Reduced emission of CO2 about 36% compared to the previous model.(AQ2200-242)
Results of Life Cycle Assessment.

 

AQ9340 MPO connector adapter

- Applicable connector:
12-fiber or 24-fiber (AQ9340-12)
16-fiber or 32-fiber (AQ9340-16)*1
- Compatible with both with and without guide pins
- Applicable fiber SM(9.5/125µm)*2 , GI(50/125µm)

- Applicable sensor:
AQ2200-232 Optical Sensor Head (Large diameter detector, 800 to 1700 nm),
AQ2200-242 Optical Sensor Head (Large diameter detector, 400 to 1100 nm)


*1 The AQ9340-16 can only be used with AQ2200-242.
*2 AQ9340-12.

AQ9436C Ribbon fiber adapter

- Adapter for a ribbon fiber folder of fusion splicer
- Fiber count: 2, 4, 8 and 12 fibers
- Applicable fiber
SM(9.5/125µm), GI(50/125µm)
- Applicable sensor:
AQ2200-232 Optical Sensor Head (Large diameter detector, 800 to 1700 nm),
AQ2200-242 Optical Sensor Head (Large diameter detector, 400 to 1100 nm)

AQ9335C(FC) Connector Adapter for optical sensors

FC connector, for optical sensors
(A light shielding cap is not included)

AQ9335C(SC) Connector Adapter for optical sensors

SC connector, for optical sensors
(A light shielding cap is not included)

AQ9335C(LC) Connector Adapter for optical sensors

LC connector, for optical sensors
(Dust protection cap is not included)

AQ9335C(MU) Connector Adapter for optical sensors

MU connector, for optical sensors
(Dust protection cap is not included)

M3407HA Light shielding cap (FC)

Light shielding cap for FC connector

M3407HB Light shielding cap (SC)

Light shielding cap for SC connector

M3407HD Dust protection cap (LC)

Dust protection cap for LC connector

M3407HE Dust protection cap (MU)

Dust protection cap for MU connector

Overview:

Lack of reliable high-speed internet access in rural regions, due to complicated logistics and the considerable costs involved to extend land-based networks to these areas, has inspired a wave of next-generation applications that will provide greater accessibility and reliability. Making use of “space laser” networks, these revolutionary solutions can relay digital traffic via low Earth orbit (LEO) satellite systems to provide low-latency, high-speed broadband services to communities typically beyond the reach of standard wireless and fiber networks.

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