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Published on: July 30, 2020
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Accelerating Faceting Wide-Field Imaging Algorithm with FPGA for SKA Radio Telescope as a Vast Sensor Array
Yuefeng Song1, Yongxin Zhu1,2,3, Tianhao Nan1
1School of Microelectronics, Shanghai Jiao Tong University, Shanghai 200240, China.
Sensors (Basel, Switzerland)
|July 26, 2020
Summary
Field-Programmable Gate Arrays (FPGAs) accelerate the faceting algorithm for the Square Kilometer Array (SKA) radio telescope. This hardware acceleration significantly boosts performance for crucial phases like phase rotation and gridding.
Area of Science:
- Astronomy and Astrophysics
- Computer Engineering
- High-Performance Computing
Background:
- The Square Kilometer Array (SKA) requires advanced algorithms like faceting for image construction from vast sensor data.
- Traditional computing struggles with the immense computational demands of SKA's wide-field imaging, particularly when accounting for Earth's curvature.
Purpose of the Study:
- To design and implement a high-efficiency Field-Programmable Gate Array (FPGA)-based hardware accelerator for the faceting algorithm in the SKA.
- To address the computational bottlenecks in the phase rotation and gridding phases of the faceting algorithm.
Main Methods:
- Algorithm analysis to identify performance bottlenecks in phase rotation and gridding.
- Optimization of memory architecture and computing logic for FPGA implementation.
- Design and simulation of loop unrolling and pipelining microstructures for the gridding accelerator.
Main Results:
- Achieved a 20x acceleration for phase rotation compared to previous work.
- Demonstrated a 5.48x acceleration ratio for gridding compared to software implementations.
- Validated the high-performance acceleration of the faceting algorithm on FPGAs.
Conclusions:
- FPGA-based hardware acceleration provides a viable solution for meeting SKA's computational constraints.
- The optimized FPGA design significantly enhances the efficiency of the faceting algorithm for radio astronomy applications.
- This approach enables high-performance image construction for vast sensor arrays like the SKA.

