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Fig. 4. | Earth, Planets and Space

Fig. 4.

From: Toward generalized planetary stereo analysis scheme—Prototype implementation with multi-resolution Martian stereo imagery

Fig. 4.

Stereo DTM assessments compared with MOLA spots. The upper arrowed lines used for the assignment of employed DTMs for the profiling. Note that the red arrowed line indicates the HiRISE DTM used for the comparison. (a) MOLA track profiling with stereo DTM over Eberswalde cater (mean value of MOLA-CTX height difference: 9.9 m, standard deviation (Std. Dev.) of height difference: 28.8 m) left for track 1 and right for track 2 respectively. (b) MOLA track profiling with stereo DTM over Warrego Valles (mean value of MOLA-CTX height difference: 15.4 m, Std. Dev. of height difference: 32.8 m) left for track 1 and right for track 2 respectively. (c) MOLA track profiling with stereo DTM over Elysium Planitia (mean value of MOLA-CTX height difference: 3.2 m, Std. Dev. of height difference: 5.5 m after surface matching, mean value of MOLA-CTX height difference: 5.4 m, Std. Dev. of height difference: 10.2 m before surface matching), left for track 1 and right for track 2 respectively.

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