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.
| Exposure of Layered Sequence in Terby Crater: ESP_013160_1530 ESP_074031_1530 (Interval in Earth days: 4743) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 74.0 | -8.4 | 2.702 | 41.5 | 52.0 |
| Differential Erosion of Light-Toned Stratigraphy in Melas Chasma: ESP_013640_1710 ESP_012928_1710 (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 | -8.93 | 285. | 8.51 | -10.3 | 39.1 | 48.9 |
| 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 |
| 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 |
| 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 |
| Sinuous Ridges in Northeast Meridiani Planum: ESP_012648_1815 ESP_012714_1815 (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 | 1.393 | 7.67 | 2.83 | -19.9 | 54.9 | 56.1 |
| 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 |
| Gullies and Light-Toned Layers in Crater Walls in Terra Cimmeria: ESP_013328_1410 ESP_014185_1410 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.6 | 168. | -6.9 | 18.35 | 39.9 | 37.0 |
| 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 |
| Exposure of South Polar Layered Deposits with Minor Faulting: ESP_012855_1065 ESP_012723_1065 (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 | -73.2 | 132. | -7.1 | 7.21 | 58.4 | 58.8 |
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