Oxford University is designing the electronics that will turn signals from 250,000 radio antennas into hundreds of steerable 'virtual dishes' for the Square Kilometre Array (SKA), the world’s largest radio telescope. This matters because the SKA will detect faint cosmic signals—from pulsars, distant galaxies, and the early universe—that current telescopes cannot see. The sheer volume of data, far beyond what existing systems can handle, requires entirely new signal processing hardware and software. Oxford is leading the hardware design for the Low-Frequency Aperture Array in Australia, and contributing to the central signal processing and science data processing systems that will combine signals, search for transient events, and automatically produce usable data products for astronomers worldwide. If successful, the SKA will transform our understanding of galaxy formation, dark energy, and the origins of stars. This is primarily fundamental science—curiosity-driven exploration of the cosmos. However, the work is done in collaboration with UK companies developing state-of-the-art signal processing systems, which could find applications in fields such as telecommunications, radar, and medical imaging—much as earlier radio astronomy research led to advances in Wi-Fi and satellite communications.
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The Square Kilometre Array is a large international project to design and build the world's largest radio telescope. It will consist of three arrays of antennas: SKA-Mid, consisting of 250 dish antennas, in South Africa; SKA-Survey, a smaller dish array in Australia; and the Low-Frequency Aperture Array (LFAA), also in Australia. This grant supports the contribution of Oxford University to three of the consortia which are developing the detailed design of the SKA. The LFAA is one of the major elements of the SKA, comprising an array of 250,000 antennas working at frequencies up to 350 MHz (similar to FM radio). Oxford is leading the design of the hardware that will process the signals from these antennas and combine them in to many hundreds of 'virtual dishes', that can be pointed and steered electronically. In the Central Signal Processing consortium, we are designing the electronics that will combine the signals from these virtual dishes to form images, and also working on the systems that will search the signals from the LFAA and the dish arrays for transient and repeating signals, such as those from pulsars. In the Science Data Processor consortium we are developing software systems that will process the huge amounts of data coming out of the SKA, automatically producing science data products that astronomers can use, and storing and disseminating these data around the world. Much of the work, particularly in the hardware design, is being done in collaboration with UK companies who will also benefit from this research as they help us to develop state-of-the-art signal processing systems, which can have applications in many fields outside of radio astronomy.
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