A martian case study of segmenting images automatically for granulometry and sedimentology, Part 1: Algorithm

被引:10
|
作者
Karunatillake, Suniti [1 ]
McLennan, Scott M. [2 ]
Herkenhoff, Kenneth E. [3 ]
Husch, Jonathan M. [4 ]
Hardgrove, Craig [5 ]
Skok, J. R. [1 ]
机构
[1] Louisiana State Univ, Baton Rouge, LA 70803 USA
[2] SUNY Stony Brook, Dept Geosci, Stony Brook, NY 11794 USA
[3] US Geol Survey, Astrogeol Sci Ctr, Flagstaff, AZ 86001 USA
[4] Rider Univ, Dept Geol Environm & Marine Sci GEMS, Lawrenceville, NJ 08648 USA
[5] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA
关键词
Mars; surface; DETERMINING GRAIN-SIZE;
D O I
10.1016/j.icarus.2013.10.001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In planetary exploration, delineating individual grains in images via segmentation is a key path to sedi-mentological comparisons with the extensive terrestrial literature. Samples that contain a substantial fine grain component, common at Meridiani and Gusev at Mars, would involve prohibitive effort if attempted manually. Unavailability of physical samples also precludes standard terrestrial methods such as sieving. Furthermore, planetary scientists have been thwarted by the dearth of segmentation algorithms customized for planetary applications, including Mars, and often rely on sub-optimal solutions adapted from medical software. We address this with an original algorithm optimized to segment whole images from the Microscopic Imager of the Mars Exploration Rovers. While our code operates with minimal human guidance, its default parameters can be modified easily for different geologic settings and imagers on Earth and other planets, such as the Curiosity Rover's Mars Hand Lens Instrument. We assess the algorithm's robustness in a companion work. (C) 2013 Elsevier Inc. All rights reserved.
引用
收藏
页码:400 / 407
页数:8
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