Extreme Data-rate Scheduling for the Data Center

Designing scalable and cost-effective data center interconnect architectures based on electrical packet switches is challenging. To overcome this challenge, researchers have tried to harness the advantages of optics in data center environment. This has resulted in exploration of hybrid switching architectures that contains an optical circuit switch to serve long bursts of traffic along with an electrical packet switch serving short bursts of traffic. The performance of such hybrid switching architectures in data center is dependent on the schedulers. Building hybrid schedulers is challenging because of varying properties of data center traffic, increasing network demands, requirements imposed by hybrid network architecture etc. Slow schedulers can negatively impact the performance of the data center network because of poor resource utilization. With future demands, this problem is going to escalate motivating the need for faster schedulers. One approach to do this would be to use a hardware based scheduler. In this paper we propose a framework that can be used to explore and evaluate hardware based hybrid schedulers.This project is supported by the EPSRC INTERNET Project EP/H040536/1.This is the author accepted manuscript. The final version is available from ACM via http://dx.doi.org/10.1145/2785956.279001

NetFPGA - Rapid prototyping of high bandwidth devices in open source

The demand-led growth of datacenter networks has meant that many constituent technologies are beyond the budget of the wider community. In order to make and validate timely and relevant new contributions, the wider community requires accessible evaluation, experimentation and demonstration environments with specification comparable to the subsystems of the most massive datacenter networks. We demonstrate NetFPGA SUME, an open-source FPGA-based PCIe board for rapid prototyping of high bandwidth devices. NetFPGA SUME has I/O capabilities for 100Gbps operation as a networking device, computing unit, or for test and measurement.This work was jointly supported by EPSRC INTERNET Project EP/H040536/1, National Science Foundation under Grant No. CNS-0855268, and Defense Advanced Research Projects Agency (DARPA) and Air Force Research Laboratory (AFRL), under contract FA8750-11-C-0249. The views, opinions, and/or findings contained in this report are those of the authors and should not be interpreted as representing the official views or policies, either expressed or implied, of the National Science Foundation, Defense Advanced Research Projects Agency or the Department of Defense. The Xilinx XUP program has been a long-standing supporter of NetFPGA and the NetFPGA SUME project is only possible with their generous support. We thank the people at Digilent Inc. We thank Micron and Cypress Semiconductor for their generous part donations.This is the author accepted manuscript. The final version is available from IEEE via http://dx.doi.org/10.1109/FPL.2015.729396

ALMA long baseline phase calibration using phase referencing

© 2016 SPIE.The Atacama Large Millimeter/submillimeter Array (ALMA) is the world's largest millimeter/submillimeter telescope and provides unprecedented sensitivities and spatial resolutions. To achieve the highest imaging capa- bilities, interferometric phase calibration for the long baselines is one of the most important subjects: The longer the baselines, the worse the phase stability becomes because of turbulent motions of the Earth's atmosphere, es- pecially, the water vapor in the troposphere. To overcome this subject, ALMA adopts a phase correction scheme using a Water Vapor Radiometer (WVR) to estimate the amount of water vapor content along the antenna line of sight. An additional technique is phase referencing, in which a science target and a nearby calibrator are observed by turn by quickly changing the antenna pointing. We conducted feasibility studies of the hybrid technique with the WVR phase correction and the antenna Fast Switching (FS) phase referencing (WVR+FS phase correction) for the ALMA 16 km longest baselines in cases that (1) the same observing frequency both for a target and calibrator is used, and (2) higher and lower frequencies for a target and calibrator, respectively, with a typical switching cycle time of 20 s. It was found that the phase correction performance of the hybrid technique is promising where a nearby calibrator is located within roughly 3? from a science target, and that the phase correction with 20 s switching cycle time significantly improves the performance with the above separation angle criterion comparing to the 120 s switching cycle time. The currently trial phase calibration method shows the same performance independent of the observing frequencies. This result is especially important for the higher frequency observations because it becomes difficult to find a bright calibrator close to an arbitrary sky position. In the series of our experiments, it is also found that phase errors affecting the image quality come from not only the water vapor content in the lower troposphere but also a large structure of the atmosphere with a typical cell scale of a few tens of kilometers