As I wrote in the last post, I am in the process of dividing up my QGIS projects covering the Mars Express HRSC DTM tiles that cover areas where Colin Souness found 'glacier-like forms' in his PhD and 
research paper.
I now come to the southeastern highlands:
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| Again, I use the equicylindrical projection optimised for 40° latitude, units are metres. | 
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| The elevation colour ramp for the underlying backdrop of the MOLA/MGS topography. In the above rendering this is blended with the Mars Orbiter Camera image mosaic. | 
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| In this region, I am able to use a single colour ramp for all of the various HRSC DTM tiles. | 
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| The MOLA elevation alone. | 
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| The MOLA elevation, blended with hillshade. | 
There are relatively few Souness GLFs in this region,found in crater walls. There are a number of these that look quite interesting - where within the same crater part of it looks glacial, and other parts have terrain produced by erosion by liquid.
Crater at 125°E, 41°S 
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| Several Souness GLFs, including one covered by an anaglyph ESP_022494_1385. | 
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| The classifier results (blue for topographic similarity to 'extent' areas, and red for topohgraphic similarity to 'head' area) overplotted on the HRSC nadir image. | 
Crater at 126°E, 44°S
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| Several Souness GLFs and other areas showing flow features. Souness 928 appears to have its 'head' and 'terminus' locations interchanged in the catalog. | 
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| Classifier results. | 
Crater at 141°E, 40°S
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| Souness 915 appears in the northern wall of the crater, and fluvial-like channels in the south wall. | 
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| A closer look at the north wall. | 
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| The classifier results. | 
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| The channels visible in the southern wall. | 
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| Classifier results. | 
Crater at 169°E, 45°S 
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| Four Souness GLFs are found in this crater. | 
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| With the classifier results. |