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.
| Terrain Northwest of Hellas Planitia: ESP_019543_1465 ESP_019899_1465 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.1 | 50.7 | 0 | 11.96 | 68.5 | 64.4 |
| Channels and Vents in Tharsis Region: ESP_019483_2010 ESP_019549_2010 (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 | 20.54 | 241. | 2.59 | -17.9 | 50.9 | 53.1 |
| Fresh 3-Kilometer Diameter Crater in Terra Sabaea: ESP_019544_1675 ESP_020177_1675 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 20.1 | 7.71 | -6.37 | 58.0 | 56.7 |
| Light-Toned Outcrops in Noctis Region: ESP_019324_1725 ESP_019469_1725 (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 | -7.62 | 266. | -5.6 | 11.59 | 57.6 | 56.1 |
| Ismenius Cavus: ESP_019333_2140 ESP_019478_2140 (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 | 33.77 | 16.9 | -14. | -2.15 | 51.9 | 52.3 |
| Western Half of Crater in Sinus Sabaeus: ESP_019307_1715 ESP_019808_1715 (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 | -8.50 | 12.3 | -21. | 6.908 | 59.3 | 56.0 |
| Fissures in Tempe Terra: ESP_019508_2245 ESP_019574_2245 (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 | 43.91 | 276. | -3.8 | -18.2 | 55.2 | 57.3 |
| Wavy Stratification Features in Crater Wall in MOC Image S14-00005: ESP_019558_1800 ESP_020125_1800 (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 | 0.165 | 357. | -10. | 0.304 | 55.2 | 54.8 |
| Cones in Isidis Planitia: ESP_019291_1965 ESP_019924_1965 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.59 | 82.7 | 17.0 | 3.208 | 48.8 | 54.0 |
| Pit on the Eastern Flank of Pavonis Mons: ESP_019351_1795 ESP_019984_1795 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.45 | 248. | -2.8 | -17.6 | 54.7 | 56.1 |
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