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Signal Processing Ambitions for DSN Radio Astronomy Tom Kuiper JPL - Caltech. NASA DSN Radio Astronomy. NASA DSN Radio Astronomy DSN Station Locations. NASA DSN Radio Astronomy Goldstone – Madrid - Canberra. Radio Astronomy Receivers 18.0 – 26.5 GHz (70-m antennas)
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Signal Processing Ambitions for DSN Radio Astronomy Tom Kuiper JPL - Caltech NASA DSN Radio Astronomy
Radio Astronomy Receivers 18.0 – 26.5 GHz (70-m antennas) 39 – 50 GHz (Madrid 34-m) 31 – 34 GHz (Goldstone 34-m) NASA DSN Radio Astronomy • Standard Receivers • 1.6 – 1.7 GHz (70-m antennas) • 2.2 – 2.3 GHz • 8.2 – 8.6 GHz • 31.5 – 32.5 GHz (not 70-m antennas)
NASA DSN Radio Astronomy • Data recorders (Standard DSN equipment) • MkV VLBI (500 MHz BW, post real-time processing) • VLBI Science Receivers ( 4x16 MHz BW, near real-time software PFB, FFT, AC) • Autocorrelators (Spaceborne) • Canberra (400 MHz, 4096 ch) • Madrid (500 MHz, 1024 ch) • Goldstone (500 MHz, 1024 ch)
NASA DSN Radio Astronomy Current Research • Extragalactic water masers (wide bandwidth, high resolution, [two polarizations]) • H20, NH3 (three lines), CCS [,C3H2] in star forming regions • CCS 11 GHz Zeeman effect in pre-protostellar clouds • VLBI • SETI
NASA DSN Radio AstronomyFuture Capability • Search for extragalactic water masers: two polarization beamswitching (four IFs) with 8192 ch over 400 MHz • Search for RRATs and isolated bursts (400 MHz BW real-time de-dispersion and capture) • Giant nanosecond pulses between 18 and 26 GHz, full Stokes (de-dispersion and capture) • Monitor Mars electrostatic microdischarges
NASA DSN Radio AstronomySignal Processing Roadmap • 08Q4 • ROACH with 1 ADC prototype development • Repair and deploy 128M ch SETI spectrometer • 09Q1-2 • Deploy and field test prototype at Goldstone • 09Q3-4 • Deploy one ROACH to each station • 10Q1 ff .....