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Martian Sonic Anemometer. D. Banfield (PI - Cornell) R. Dissly (Ball Aerospace) M. Richardson, I. McEwan (CIT) D. Schindel (MicroAcoustics). Measures wind speed via sound pulse travel-time differences. Temperature is inferred from sound speed. How to Improve Martian Wind Measurements?.
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Martian Sonic Anemometer • D. Banfield (PI - Cornell) • R. Dissly (Ball Aerospace) • M. Richardson, I. McEwan (CIT) • D. Schindel (MicroAcoustics)
Measures wind speed via sound pulse travel-time differences. Temperature is inferred from sound speed. How to Improve Martian Wind Measurements? • Adapt premier terrestrial technique for Mars: Sonic Anemometry Terrestrial Research-Grade Sonic Anemometer
Sonic Anemometry Advantages • 3-D capable (open sensing volume) • Higher sensitivity (<5 cm/s) • Higher time resolution (10-100 Hz) • Also yields temperature! (<0.2K) • OR if T provided, yields γR*/m • Improved accuracy (fewer biases) • e.g., Insensitivity to radiative heating • Resolve eddies, measure fluxes (heat, momentum, water vapor)
Why Are These Capabilities Important? • Opens up Boundary Layer studies • e.g., Test Businger-Dyer relation @ Mars! • Directly measure fluxes • Heat flux for surface energy balance • Momentum flux for aeolian processes • Water vapor flux for water stability/climate • Provide more robust measures for model validation • U, V, T, P alone aren’t enough to validate mesoscale models adequately • Fluxes give more dimensions to compare models to data • Improved models mean safer S/C delivery • Hunt critters tracking bio-tracer effluents? • Earth animals use this (hunting lobsters, mating moths)
Development History • PIDDP funding from ‘02-’06 • Proof of concept up through breadboard • Chamber tested to function @ <~4mbar CO2, -30C • Transducer miniaturization • Signal Processing algorithms explored • Stratospheric balloon flight attempted
Development Challenges CO2 attenuates high frequencies • High frequencies critical for precise timing • Answers: • Broadband transducers • Good signal processing • -e.g., Pulse compression (from radar), spread spectrum (cell phones), Kalman Filtering From Williams (2000)
Development Challenges Emitting/Receiving Sound in 6 mbar CO2 • Low atm density means poor transducer coupling • Acoustic impedance mismatch using piezoelectric devices in low pressure medium • Answer is to useappropriate transducers: Capacitive micro-machined devices
Metal contact (fixed backplate) Metal contact (movable) Silicon nitride membrane Etch Holes Air cavity Insulator Substrate 1mm Capacitive Transducers
Capacitive Transducers Developed new Miniature Transducers for Anemometer Use • 1.1cm diameter X 0.7cm depth
Notional System for Flux Measurements Combine with TDL hygrometer for water flux • TDL Hygrometer adds about 500g, 256cm3 • Sensitivity of 0.1ppmv at 10 Hz (Webster, personal comm.) • Should be sufficient for measuring typical Martian water vapor regolith/atmospheric exchange in real time
Martian Sonic Anemometer • Technical Characteristics: • Mass: 950 g • Volume: Total: 1500 cm3 • electronics: 1000 cm3 • Sensor Head: D=15 cm sphere deployed D=15 cm X 3 cm deep cylinder stowed • Power: <10 W active, 0 W quiescent • On-time: instantaneous • Maximum Data Rate: 1200 Byte/s • Typical Data Rate: 80 Byte/s • Typical observing scenario: 2 min every 2 hours => 4 W-hr/day & ~0.1 MB/day • Key Performance Characteristics: • Measurement Rate: <100 Hz • Wind Speed Accuracy: ~<5 cm/s • Temperature Accuracy: 0.2 K • Fluxes (horizontal and vertical; heat, momentum, water vapor?)
Acoustic anemometer measures wind via sound pulse travel-time differences. Temperature is measured from average travel times. Scout Sonic Anemometer • PI- Don Banfield (Cornell) • The Mars Sonic Anemometer uses earth-proven techniques with Mars-specific micro-machined acoustic transducers. • Measures 3-D wind vector and co-located temperature, and resolves turbulent eddies. • 3-D measurement means deployment insensitive. • Combined with TDL hygrometer, can return water vapor flux; but alone can still return heat and momentum fluxes Deployable Mast Sensor Array (15 x 15 x 3cm stowed) Electronics Box
Status and Future Work • Currently TRL~4 for system • PIDDP funding from ’09-’11 • Transducer optimization • Tune for typical s/c voltage operation • Transducer environmental validation • Test at LOW temps & high thermal cycling • Test under dust impact exposure • Electronics miniaturization/optimization • Flight-like electronics • Field/Wind Tunnel/Stratospheric Balloon Testing • Test against terrestrial standards • Test at Ames MARSWIT • Test on Stratospheric Balloon