1. Characterization of the electro-optical transceivers in the KM3NeT optical network S.Pulvirenti, F. Ameli, A. D’Amico, G. Kieft, J-W Schmelling for KM3NeT Collaboration 15-09-2015 1

2. Summary 2 Introduction The electro-optical transceiver in KM3NeT OESolution SFP Transceiver Wavelength tuning (First) Tests at Nikhef Device aging and wavelength drift Test bench Test Procedure Preliminary results Conclusion and future Test

3. Introduction 3 The presentation shows preliminary results about the characterization of the tuneable features of the electro-optical transceivers used in KM3NeT network. Over the telescope life time, precise temperature control of the laser is required to maintain stability of the central frequency, complying with the ITU-T G.694.1 recommendations of the International Telecommunication Union. This characterization is required to compensate for the expected wavelength drift due to aging factors.

4. SFP Transceivers in KM3NeT 4 They are a key element in the KM3NeT network, present in DOM, JB, Tower Floor, Shore Station

5. OESolution SFP Transceivers The data transport over the KM3NeT optical network is based on the Dense Wavelength Division Multiplexing (DWDM) technique with optical channels spaced 50 GHz apart, a bit rate of 1.25Gbps and up to 100 km span length. 5 The digital diagnostic monitoring interface allows real time access to the device operating parameters: Transmitted Optical Power Received Optical Power Transmitter Bias Current Transceiver Temperature Laser Temperature Supply Voltage TEC Current KM3NeT SFP Requirements

6. Wavelength tuning 6 The wavelength tuning feature of a SFP is a special feature which is not required by the DWDM SFP MSA standards. The principle of the wavelength tuning is based on changing the temperature of the TOSA (Transmission Optical SubAssembly). To be more precise change the temperature of the laser cavity. Inside a SFP there is a temperature control circuitry which on its turn is connected to a microcontroller. The actual change of temperature is done via a TEC (Thermoelectric cooling) controller. This TEC controller on its turn is connected to the microcontroller where it gets its set-point from. The actual wavelength tuning by the user is done by changing data in the microcontroller memory which is translated to the temperature setting of the TEC and thus the TOSA temperature. All the communication is done via the I2C bus of the SFP transceiver. The expected wavelength change is typically 100 pm/°C

7. (First) Tests at Nikhef 7 Wavelength measurements at Nikhef performed using an Ando wavelength meter, model model AQ6140, instead of an OSA. Main specifications: Wavelength range 1270 to 1650 nm Wavelength accuracy ±2 ppm (1550 nm, 1310 nm: ±0.003 nm) Minimum resolvable seperation 10 GHz or less (1550 nm: 80 pm, equal power line input)

8. DAC offset vs Wavelength change 8 DAC variationMax variation -100pm6% +100pm10%

9. Wavelength tuning response 9

10. Device aging and wavelength drift 10 Over the device lifetime, the laser diode will exhibit wavelength drift. Eventually the wavelength drift could drive the channel into the neighbouring one then disrupting the communication.

11. uBlaze I2C RS232 SFP Laser Xilinx Spartan6 - FPGA FCM Board Test Bench Communicate with Host PC (RS232) Optical Spectrum Analyzer A MicroBlaze microcontroller is embedded in the FCM FPGA: Soft IP core (synthesizable); Xilinx development environment; Peripheral availability for standard communication protocol with drivers and APIs; A dedicated SW has been written to: read/write Laser registers (I2C); implement tuning procedure for OESolutions Laser; communicate with Host PC (RS232);

12. Test bench tools 12 OSA – Optical Spectrum Analyzer: Wavelength range [nm] 1250 to 1650 Resolution bandwidth FWHM 0.065 nm Wavelength uncertainty [nm] ± 0.05 Wavelength repeatability [nm] ± 0.003 Wavelength linearity [nm] typical ± 0.01 FCM – Floor Control Module is KM3NeT-IT Floor Control Module: Communication with On-Shore through SFP Laser; - Use of Custom Protocol Collection of digital streams from 6 PMTs located in the Optical Modules; Collection of data from 2 hydrophones; Communication with floor oceanographic instrument Management of local sensors (Temperature, Relative Humidity, Currents and Voltages, etc.) See Carlo Nicolaus’s Talk

13. Test Procedure 13 Warm up time: > 15 minutes Initial settings of the transceiver: Factory settings Disable the transceiver alarms Store the factory tuning value Temperature scan 2°C Wavelength scan: -Acquisition of factory settings -Four samples before scan start (at nominal wavelength) -Eight samples during the wavelength scan. -Four samples after scan stop (at nominal wavelength)

14. Preliminary results (over 8 scan samples) 14 Wavelength vs Laser temperature

15. Preliminary Results (Linear Fit) 15 Example CH 30C (λ = 1553,33 nm)

16. 16 Preliminary results – CH 59C λ = 1530,33 nm Factory settings (4 samples scan) Factory settings (4 samples scan)

17. 17 Preliminary results – CH 59C Linear fit between Laser temperature and Tuning Value

18. Conclusion and Future Test 18 Aging stress test – Monitor the SFP behavior in a long period and check the center wavelength stability at high temperature Accumulate more statistics (more devices of the same wavelength) Characterize more devices covering the whole C band within ± 100 pm from the nominal wavelength Aim to predict the correction to be applied in case of a drift of more than ± 50 pm

19. 19 Thank you for your attention!