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arXiv 2103.09673astro-ph.IMastro-ph.EPcs.LG
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Automatic detection of impact craters on Al foils from the Stardust interstellar dust collector using convolutional neural networks

Space Sciences Laboratory, University of California at Berkeley(加州大学伯克利分校空间科学实验室);Centre for Astrophysics and Planetary Science, University of Kent(肯特大学天体物理与行星科学中心);Washington University(华盛顿大学)
Logan Jaeger, Anna L. Butterworth, Zack Gainsforth, Robert Lettieri, Augusto Ardizzone, Michael Capraro, Mark Burchell, Penny Wozniakiewicz, Ryan C. Ogliore, Br… 展开作者

Logan Jaeger, Anna L. Butterworth, Zack Gainsforth, Robert Lettieri, Augusto Ardizzone, Michael Capraro, Mark Burchell, Penny Wozniakiewicz, Ryan C. Ogliore, Bradley T. De Gregorio, Rhonda M. Stroud, Andrew J. Westphal

英文摘要:

NASA's Stardust mission utilized a sample collector composed of aerogel and aluminum foil to return cometary and interstellar particles to Earth. Analysis of the aluminum foil begins with locating craters produced by hypervelocity impacts of cometary and interstellar dust. Interstellar dust craters are typically less than one micrometer in size and are sparsely distributed, making them difficult to find. In this paper, we describe a convolutional neural network based on the VGG16 architecture that achieves high specificity and sensitivity in locating impact craters in the Stardust interstellar collector foils. We evaluate its implications for current and future analyses of Stardust samples.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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