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.
| North Wall of Ritchey Crater: ESP_013125_1520 ESP_013758_1520 (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 | -27.9 | 309. | 0.17 | -22.9 | 41.2 | 37.0 |
| Lobate Features in the Charitum Montes: ESP_013165_1275 ESP_013244_1275 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -51.9 | 301. | -4.0 | 20.40 | 45.0 | 42.6 |
| Well-Preserved Large Crater West of Elysium Region: ESP_013567_2035 ESP_021571_2035 (Interval in Earth days: 624) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.31 | 114. | 5.79 | 18.66 | 59.6 | 63.4 |
| Edge of Fluidized Ejecta Rampart with Great Phyllosilicate Signature: ESP_012909_1680 ESP_013331_1680 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.9 | 83.6 | 3.17 | -12.0 | 47.1 | 43.1 |
| Aram Chaos: ESP_013783_1820 ESP_022486_1820 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.171 | 339. | 7.62 | -21.2 | 42.9 | 44.4 |
| Well-Preserved Gullied Impact Crater: ESP_013962_1430 ESP_021676_1430 (Interval in Earth days: 601) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.7 | 138. | 0.22 | -12.7 | 36.6 | 43.8 |
| Crossing Wrinkle Ridges in Tyrrhena Dorsa: ESP_012631_1555 PSP_005234_1555 (Interval in Earth days: 576) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.1 | 115. | -1.3 | 17.00 | 48.2 | 31.9 |
| 10 Kilometer Diameter Rayed Crater: ESP_012738_1785 ESP_013094_1785 (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 | -1.41 | 70.8 | 2.49 | 14.97 | 53.0 | 48.7 |
| Possible Sulfates in Ius Chasma: ESP_013759_1720 ESP_020550_1720 (Interval in Earth days: 529) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.88 | 276. | 4.68 | -17.6 | 38.5 | 55.9 |
| Dark Deposits in Gullies in Ariadnes Colles: ESP_013341_1455 ESP_013763_1455 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.3 | 172. | 2.11 | -11.4 | 38.6 | 36.8 |
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