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.
| Gullies in Light-Toned Rock: ESP_012795_1395 ESP_013507_1395 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.2 | 319. | 2.74 | 16.59 | 45.9 | 37.2 |
| Ejecta Falling Into Earlier Large Crater: ESP_013346_1940 ESP_013768_1940 (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 | 13.86 | 29.4 | 6.71 | -7.95 | 55.5 | 51.3 |
| Well Preserved 20 Kilometer Diameter Impact Crater: ESP_013684_1455 ESP_020910_1455 (Interval in Earth days: 563) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 168. | -2.8 | 19.71 | 36.4 | 51.7 |
| Fretted Terrain-Like Aprons Near Reull Vallis: ESP_012935_1415 ESP_013212_1415 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.2 | 96.9 | 6.90 | -17.4 | 43.4 | 41.9 |
| Layered Bedrock in Northeast Hellas Planitia: ESP_013964_1490 ESP_020267_1490 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.7 | 82.9 | 1.84 | 19.77 | 34.9 | 58.9 |
| Exposure of Layers in South Gale Crater with Possible Sulfates: ESP_014186_1745 ESP_020410_1745 (Interval in Earth days: 485) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.56 | 138. | 8.10 | -13.1 | 35.2 | 55.9 |
| Channel Carved Into Scarp within Isidis Planitia: ESP_013186_1945 ESP_013252_1945 (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 | 14.55 | 78.4 | -2.7 | -24.1 | 58.1 | 58.9 |
| Western Half of Very Well-Preserved Gullied Crater: ESP_012807_1505 ESP_012952_1505 (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 | -29.4 | 351. | -5.9 | 9.919 | 45.8 | 42.6 |
| Saheki Crater Alluvial Fan Layering Exposed in Eastern Portion of Crater: ESP_012949_1580 ESP_013226_1580 (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 | -21.7 | 73.0 | 0.82 | -26.3 | 44.2 | 42.9 |
| Ares Vallis Wall and Floor Exposures: ESP_013216_1870 ESP_022143_1870 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.694 | 340. | -2.5 | 20.39 | 53.0 | 48.5 |
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