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.
| Nili Fossae Trough, Candidate MSL Landing Site: PSP_003086_2015 PSP_003587_2015 (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 | 21.12 | 74.2 | -6.8 | 19.81 | 62.4 | 62.7 |
| Gale Crater: PSP_001554_1745 ESP_018999_1745 (Interval in Earth days: 1359) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.33 | 138. | -13. | 10.53 | 57.8 | 56.0 |
| Lots of Layering in Becquerel Crater: PSP_003656_2015 PSP_005845_2015 (Interval in Earth days: 170) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.31 | 352. | 2.46 | -21.8 | 64.2 | 45.8 |
| Layered Deposits in Terby Crater: PSP_001662_1520 PSP_002572_1520 (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 | -27.5 | 74.2 | -3.0 | -17.3 | 67.8 | 61.8 |
| Light-toned Layering on Plains South of the West Candor Region: PSP_005096_1730 PSP_005241_1730 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.93 | 283. | -12. | 2.319 | 37.7 | 35.4 |
| Flow-like Features in Promethei Terra: PSP_005419_1380 PSP_005696_1380 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.6 | 108. | -0.9 | -24.6 | 39.8 | 44.5 |
| Channels East of Olympus Mons: PSP_005401_1960 PSP_005546_1960 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.99 | 232. | -5.7 | 8.395 | 46.2 | 43.7 |
| Chain of Pits on Arsia Mons: PSP_005414_1735 ESP_011756_1735 (Interval in Earth days: 494) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.52 | 240. | 3.62 | 20.67 | 34.2 | 55.5 |
| Small Winding Channel in Tartarus Colles: PSP_001420_2045 ESP_069174_2045 (Interval in Earth days: 5279) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.47 | 188. | 7.84 | 27.97 | 47.7 | 44.4 |
| Gullies in Mantle Terrain in Sisyphi Planum: PSP_005160_1150 PSP_005595_1150 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -64.8 | 344. | 0 | 20.43 | 52.1 | 56.4 |
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