21-22 September 2020
Max Planck Institute for Radio Astronomy
Europe/Berlin timezone
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Contribution

Max Planck Institute for Radio Astronomy - Lecture Hall 0.02

Solar power mirror arrays for radio astronomy - towards a test with the Juelich Solar Power Tower

Content

We have presented the idea at past meetings to use the mirror arrays of concentrating solar power stations as vast collecting areas for high-sensitivity radio astronomy. Since the signals do not combine coherently they will produce an extended speckle pattern over the focal region that requires a large phased array feed to collect and combine in-phase. The 4000 element EMBRACE array developed under the RadioNet SKADS project is such array feed and might conceivably be re-purposed for this application. We will give an update on the idea and the plans for a proof-of-concept experiment on the Juelich experimental solar array. For simplicity these start with a two-pixel receiver before scaling up.