Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Depression Near Warrego Valles Uplands: PSP_005967_1400 ESP_059042_1400 (Interval in Earth days: 4136) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 267. | -3.4 | 7.221 | 45.5 | 45.9 |
| Alluvial Fans in Unnamed Crater: PSP_006528_1585 PSP_007095_1585 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 67.1 | 0 | -14.3 | 43.3 | 52.6 |
| Layered Bedrock Exposed in the Central Uplift of Martin Crater: PSP_005821_1585 ESP_011952_1585 (Interval in Earth days: 477) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 290. | -1.8 | 21.33 | 35.0 | 54.2 |
| Boundary of Ejecta Layers at Tooting Crater: PSP_006193_2035 PSP_007116_2035 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.02 | 208. | 0 | -13.0 | 42.2 | 40.5 |
| Floor of Ares Vallis: PSP_006940_1900 PSP_007876_1900 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.11 | 334. | -1.8 | 20.02 | 38.4 | 42.9 |
| Fresh Double-Layered Crater with Possible Ponded Materials: PSP_006945_2350 PSP_007235_2350 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.57 | 190. | 1.13 | 12.28 | 54.1 | 50.5 |
| Basal Exposure of South Polar Layered Deposits: PSP_005102_1030 PSP_005155_1030 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -76.8 | 132. | 7.05 | -13.4 | 60.2 | 62.0 |
| Seasonal Monitoring: PSP_005455_0975 PSP_005547_0975 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.1 | 225. | 1.30 | 15.98 | 69.4 | 69.9 |
| South Polar Layered Deposits Survey: PSP_005302_0880 PSP_005801_0920 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.7 | 153. | 6.38 | 18.16 | 73.1 | 78.7 |
| Gratteri Crater Continuous Ejecta Blanket: PSP_005521_1620 ESP_012786_1620 (Interval in Earth days: 566) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.6 | 200. | 3.46 | 27.99 | 32.5 | 44.9 |
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