5 Planetary Geology
Sunday, 7 November 2004
8:00 AM - 12:00 PM
UNWRAPPING THE WHIRLWIND; MEASURING NATURAL DUST DEVILS
Paper number: 5-12
Program: Technical Sessions
Time: 10:45 AM – 11:00 AM
Authors
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John ZarneckiOpen Univ, Milton Keynes, N/A
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Matt BalmeUniv College London, London, N/A
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William M. FarrellGSFC, Greenbelt, MD
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Stephen FuerstenauJPL, Pasadena, CA
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Ron GreeleyArizona State Univ, Tempe, AZ
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Jonathan MerrisonAarhus Univ, Aarhus, N/A
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Mannish PatelOpen Univ, Milton Keynes, N/A
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Timothy RingroseOpen Univ, Milton Keynes, N/A
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Martin TownerOpen Univ, Milton Keynes, N/A
Abstract
The chase rig consists of a terrain-following 5-m vertical mast supporting 30 instruments that profile wind speed, temperature, pressure, and humidity. Additional single-level instruments measure particle impacts, particle charge states, and UV insolation levels (several of which were developed for the Beagle2 Mars lander). Dust devils could not sustain their thermal engine when ambient winds dropped below 2 m/s. Conversely, vortex structure was disbursed and destroyed when ambient winds exceeded 8 m/s, although in both cases short-lived vortices could develop. Under such conditions, a dozen events were well documented by datalogger and cameras. This report will present the latest findings from the 2004 field season as we strive to assimilate these simultaneous data sets.