火星大沙波纹特征及其形成机制 |
董治宝, 吕萍, 李超, 胡光印 |
Characteristics and Formation Mechanism of Large Ripples on Mars |
Zhibao Dong, Lü Ping, Chao Li, Guangyin Hu |
图10 火星大沙波纹的纵向延伸(据参考文献[ (a)火星盖尔陨击坑拜格诺沙地大沙波纹的纵向移动(T1~T3时间段);(b)不同时期Y-结点的位置;(c)移动方向与大沙波纹走向对比;(a)和(b)中黄色、红色和蓝色线条分别代表大沙波纹在T1、T2和T3时间段的纵向移动 |
Fig.10 Longitudinal migration of LRs (modified after reference [ (a) Longitudinal migration of LRs in the Bagnold dunefield, Gale crater, Mars (at T1~T3); (b)The location of Y junction with time; (c) Comparation of longitudinal direction of Y junction and crest orientation of LRs; Yellow, red, and blue lines in figure (a) and (b) represent longitudinal migration of LRs during the period of T1, T2, and T3 |
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