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arxiv: 1706.08863 · v1 · pith:73EQV6HVnew · submitted 2017-06-27 · 🌌 astro-ph.IM · astro-ph.SR

OCTAD-S: Digital Fast Fourier Transform Spectrometers by FPGA

classification 🌌 astro-ph.IM astro-ph.SR
keywords spectrometersfpgasamplingchannelsdigitalfastfourierfrequency
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We have developed a digital fast Fourier transform (FFT) spectrometer made of an analog-to-digital converter (ADC) and a field-programmable gate array (FPGA). The base instrument has independent ADC and FPGA modules, which allow us to implement different spectrometers in a relatively easy manner. Two types of spectrometers have been instrumented, one with 4.096 GS/s sampling speed and 2048 frequency channels and the other with 2.048 GS/s sampling speed and 32768 frequency channels. The signal processing in these spectrometers has no dead time and the accumulated spectra are recorded in external media every 8 ms. A direct sampling spectroscopy up to 8 GHz is achieved by a microwave track-and-hold circuit, which can reduce the analog receiver in front of the spectrometer. Highly stable spectroscopy with a wide dynamic range was demonstrated in a series of laboratory experiments and test observations of solar radio bursts.

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