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.
| Small Fresh Primary or Large Secondary Crater From Gratteri Crater: PSP_007209_1565 PSP_008290_1565 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.3 | 194. | -6.7 | 16.15 | 54.8 | 65.4 |
| Fresh 10-Kilometer Diameter Unnamed Crater in Terra Sabaea: PSP_007966_1615 ESP_025055_1615 (Interval in Earth days: 1331) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.1 | 41.5 | 5.02 | 25.73 | 59.9 | 51.0 |
| Craters on an Ice-Rich Debris Apron: PSP_007832_1385 ESP_060736_1385 (Interval in Earth days: 4123) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.3 | 103. | 1.98 | -19.2 | 74.9 | 74.8 |
| Gullies: PSP_007456_2140 ESP_016040_2140 (Interval in Earth days: 669) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.74 | 281. | -4.6 | -22.7 | 41.7 | 43.6 |
| Unnamed Well-Preserved Crater in Terra Cimmeria: PSP_007000_1475 PSP_007145_1475 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.0 | 141. | -1.0 | 10.11 | 57.0 | 58.6 |
| Utopia Planitia Crater with Candidate Pingos: PSP_007780_2450 PSP_008492_2450 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 64.51 | 67.2 | 2.76 | -8.38 | 52.4 | 49.6 |
| Well-Peserved Large Crater with Central Peak and Pit: PSP_007366_1360 ESP_024732_1360 (Interval in Earth days: 1353) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.4 | 229. | 2.46 | -27.4 | 70.5 | 67.3 |
| Gullies as Seen in MOC Image M02-02681: PSP_007213_1400 ESP_042618_1400 (Interval in Earth days: 2759) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 86.3 | 2.71 | 26.46 | 65.4 | 65.6 |
| Small Crater with Layered Fill in Schiaparelli Crater: PSP_007400_1790 PSP_007756_1790 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.75 | 14.3 | 9.35 | -3.82 | 44.1 | 48.4 |
| Interior Channel in Durius Valles: PSP_007012_1630 PSP_007157_1630 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.8 | 171. | -3.9 | 8.48 | 48.0 | 49.2 |
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