Over several years, STAR-Dundee has developed a range of Fast Fourier Transform (FFT) based wideband spectrometers (WBS). The latest of these, WBS V, is a prototype flight board designed in a radiation tolerant FPGA, the Microsemi RTG4. Implemented in the RTG4 is a 1024-point FFT based spectrometer offering processing power in the region of 100 GOPS, enabling operation at 2.4 Gsamples/s.
On Wednesday the 5th of September 2018, STAR-Dundee will be delivering a presentation and poster at the UK National Earth Observation Conference in Birmingham, describing some of the technical details of the WBS V and the unique scientific research that it is being used to perform. The presentation is being held in Room G3 at 10:24, while the poster will be presented from 17:00 to 19:00 in the Great Hall.