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首页> 外文期刊>Earth, Moon, and Planets: An International Journal of Comparative Planetology >The Subjectivity in Identification of Martian Channel Networks and Its Implication for Citizen Science Projects
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The Subjectivity in Identification of Martian Channel Networks and Its Implication for Citizen Science Projects

机译:识别火星渠道网络的主观性及其对公民科学项目的含义

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摘要

The Martian surface is incised by numerous valley networks, which indicate the planet experienced sustained widespread flowing water in the past (e.g. Carr in Water on Mars, Oxford University Press, New York, 1996; Phil Trans R Soc A 370:2193-2212, 2012. 10.1098/rsta.2011.0500). Examining the distribution and geometries of these valley networks provides invaluable information about the Martian climate during the period of formation. The recent advancement in high resolution images has provided an opportunity to build upon past valley maps of Mars (Bahia et al. in LPSC 2018, 2018), however, the identification of these valley networks is extremely time-consuming. A citizen science project may aid in reducing this time-consuming process; this project conducts a valley mapping task with participants of varying expertise in valley mapping to determine whether a citizen science project of this kind should be worth pursuing. This was conducted in a region adjacent to Vogel Crater (36.1 degrees S, 10.2 degrees W). Repeated mapping of the area (a repeatability test) found that participants with low experience in valley mapping (22 a-level physics student's representative of the public) were inconsistent when mapping valleys. Additionally, when comparing the results of participants within this group (a reproducibility test), the majority of reproduced valleys are false positives (i.e. incorrectly traced valleys). These results were consistent with those found for the medium experience group (45 2nd year geology undergraduates). The validated tracings of the low experience group improve upon the number and total length of valleys mapped by previous studies (Hynek et al. in J Geophys Res 115:1-14, 2010). To validate these valleys requires the input of an expert to remove false positives which is less time consuming than manually mapping the images; this may indicate that a citizen science project is worth pursuing. However, to effectively identify the maximum amount of valleys an expert is required.
机译:火星表面由众多谷网络切开,这表明该行星过去经历过持久的普遍流动水(例如,牛津大学出版社,纽约,1996年牛津大学出版社的马斯在水中停用; Phil Trans R SoC A 370:2193-2212, 2012. 10.1098 / RSTA.2011.0500)。检查这些谷网络的分布和几何形状提供了有关在地层期间有关火星气候的宝贵信息。最近高分辨率图像的进步已经为火星的过去谷地图提供了机会(Bahia等人。然而,在2018年的LPSC 2018年,2018年),这些谷网络的识别是非常耗时的。公民科学项目可能有助于减少这种耗时的过程;该项目开展了谷映射任务,与Valley Mapping的不同专业知识的参与者,以确定这种情况的公民科学项目是否值得追求。这在与Vogel火山口相邻的区域中进行(36.1度,10.2°W)。对该区域的重复映射(重复性测试)发现,谷映射中具有低经验的参与者(公众的22个A级物理学生代表)在映射谷时不一致。此外,当比较该组内参与者的结果(再现性测试)时,大多数再现山谷是误报(即,追踪的山谷不正确)。这些结果与媒体经验组(第45年地质大学生)的结果一致。低经验组的验证追踪提高了以前研究的谷的数量和总长度(Hynek等人。在J Geophys Res 115:1-14,1010中)。为了验证这些valleys需要输入专家以消除比手动绘制图像的耗时少的误报;这可能表明公民科学项目值得追求。但是,为了有效地识别需要专家的最大数量。

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