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タイトルRestoration and Reexamination of Apollo Lunar Dust Detector Data from Original Telemetry Files
本文(外部サイト)http://hdl.handle.net/2060/20120009885
著者(英)Hills, H. Kent; McBride, M. J.; Williams, David R.
著者所属(英)NASA Goddard Space Flight Center
発行日2012-03-20
言語eng
内容記述We are recovering the original telemetry (Figure I) from the Apollo Dust, Thermal, Radiation Environment Monitor (DTREM) experiment, more commonly known as the Dust Detector, and producing full time resolution (54 second) data sets for release through the Planetary Data System (PDS). The primary objective of the experiment was to evaluate the effect of dust deposition, temperature, and radiation damage on solar cells on the lunar surface. The monitor was a small box consisting of three solar cells and thermistors mounted on the ALSEP (Apollo Lunar Surface Experiments Package) central station. The Dust Detector was carried on Apollo's 11, 12, 14 and 15. The Apollo 11 DTREM was powered by solar cells and only operated for a few months as planned. The Apollo 12, 14, and 15 detectors operated for 5 to 7 years, returning data every 54 seconds, consisting of voltage outputs from the three solar cells and temperatures measured by the three thermistors. The telemetry was received at ground stations and held on the Apollo Housekeeping (known as "Word 33") tapes. made available to the National Space Science Data Center (NSSDC) by Yosio Nakamura (University of Texas Institute for Geophysics). We have converted selected parts of the telemetry into uncalibrated and calibrated output voltages and temperatures.
NASA分類Lunar and Planetary Science and Exploration
レポートNOGSFC.CPR.00165.2012
権利Copyright, Distribution as joint owner in the copyright


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