国土资源遥感Issue(1)：95-99,5.DOI:10.6046/gtzyyg.2012.01.17
基于粗糙度的月表虹湾地区地形地貌解译
The Interpretation of the Land Form of Sinus Iridum on the Moon Based on the Roughness
摘要
Abstract
The planetary surface roughness is the record of erosion, deposition, uplift and other geological processes on the planetary surface, and hence serves as a prediction for the geological age of the planetary surface. In this paper, twelve profiles were selected in the horizontal direction of the Sinus Iridum in the moon, and several parameters of roughness of those profiles were studied. Some results have been obtained: d)The average of RMS height along the profile 1 km in length is about 3m. In addition, within the research scale selected in this paper (0. 2 ～ 3 km) , the slope of Sinus Iridum area does not exceed 2 °. This means that the surface of Sinus Iridum is relatively smooth. (2)Hurst exponent of Sinus Iridum is mainly concentrated from 0. 5 to 0. 78 , which means that the surface morphology is rather homogeneous. ③Low latitude areas (lower than 44. 3° N) have relatively high Hurst exponent (from 0.6 to 0. 8) , and high latitude areas (higher than 44. 3° N) usually have lower Hurst exponent ( from 0.5 to 0. 8 ). (4)The roughness may be used as a means to determine the relative geological age.关键词
虹湾/粗糙度/Hurst指数/地貌形态/相对地质年龄Key words
Sinus Iridum/ roughness/ Hurst exponent/ surface morphology/ relative geological age分类
信息技术与安全科学引用本文复制引用
奚晓旭,刘少峰,吴志远,韦蔚,焦中虎,李力..基于粗糙度的月表虹湾地区地形地貌解译[J].国土资源遥感,2012,(1):95-99,5.基金项目
国家863项目重点课题"月球数字地质图编制与月球演化模型综合研究"(编号:2009AA12220101)资助. （编号:2009AA12220101）
