2017
DOI: 10.1016/j.actaastro.2017.08.021
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Statistical multi-criteria evaluation of non-nuclear asteroid deflection methods

Abstract: This version is available at https://strathprints.strath.ac.uk/61691/ Strathprints is designed to allow users to access the research output of the University of Strathclyde. Unless otherwise explicitly stated on the manuscript, Copyright © and Moral Rights for the papers on this site are retained by the individual authors and/or other copyright owners. Please check the manuscript for details of any other licences that may have been applied. You may not engage in further distribution of the material for any pro… Show more

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Cited by 16 publications
(17 citation statements)
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References 28 publications
(32 reference statements)
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“…Hence, from both equations (13) and (14), it holds that the criteria C 7 (level of maturity) and C 4 (asteroid composition) interchange their relative level of importance from the SWAM operator to the TFS version of AHP. Specifically, it holds that C 4 appears as a more important criterion than C 7 when applying SFS TOPSIS.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Hence, from both equations (13) and (14), it holds that the criteria C 7 (level of maturity) and C 4 (asteroid composition) interchange their relative level of importance from the SWAM operator to the TFS version of AHP. Specifically, it holds that C 4 appears as a more important criterion than C 7 when applying SFS TOPSIS.…”
Section: Resultsmentioning
confidence: 99%
“…Since they are able to closely approach Earth's orbit, small perturbations regarding their orbits may place them on a collision path to the Earth. As such, to perform an exhaustive tracking of these asteroids is recommended [14,15].…”
Section: Introductionmentioning
confidence: 99%
“…For further technical details regarding each NEA deflection approach described above, we refer the reader to [8], [29], and [35].…”
Section: The Nea Deflection Alternatives Selected For Assessmentmentioning
confidence: 99%
“…根据预警时间长短以及目标小行星尺寸的不同, 主动防御技术可分为3大类 [26,27] : (1) 针对短预警时间、 大尺寸PHA, 利用核爆炸摧毁或者改变其轨道; 能够通过长期作用改变PHA的技术手段包括: 质 量驱动、拖船、太阳光压、引力牵引、激光驱动、离 子束等 [17,28] . 这些手段一般适用于防御预警几年甚至 几十年的小行星.…”
Section: 防御技术unclassified