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- W2014093313 abstract "Orbital debris objects with sizes of 6 mm and larger were detected when they passed through the main beam of the high-power, 12.6-cm wavelength radar at the Arecibo Observatory. The number of objects detected at altitudes below 1000 km in the size range of 6 mm to 2 cm agreed with orbital debris model predictions to better than a factor of two. Radar detections of larger orbital debris (10-cm diameter and above) were also compared with the objects in the U.S. Space Command catalog (the cataloged objects have UHF radar cross-sections larger than 0.01 sq m). This experiment demonstrated that the large, earth-based radar telescopes normally used for planetary studies can provide useful data about the near-earth orbital debris populations." @default.
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- W2014093313 date "1992-02-07" @default.
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- W2014093313 title "Radar detection of centimeter-sized orbital debris: Preliminary Arecibo observations at 12.5-CM wavelength" @default.
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- W2014093313 doi "https://doi.org/10.1029/91gl02772" @default.
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