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.
| Small Pedestal Crater on Ejecta of Larger Craters: ESP_032961_1385 ESP_033251_1385 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.9 | 206. | -1.0 | 18.10 | 54.6 | 58.4 |
| Tilted Layers in Center of Oudemans Crater: ESP_033275_1700 ESP_033697_1700 (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 | -9.92 | 268. | 8.73 | -8.81 | 40.6 | 47.1 |
| Stratigraphic Relation between Gully Aprons and Dunes: ESP_033120_1205 ESP_032896_1205 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -58.9 | 183. | 28.3 | 4.079 | 69.3 | 66.7 |
| Ridges in Meridiani Planum: ESP_033206_1800 ESP_033496_1800 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.069 | 351. | 0.89 | 27.28 | 37.3 | 37.8 |
| Crater on the Northern Plains: ESP_032904_2300 ESP_033181_2300 (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 | 49.41 | 309. | 4.58 | -17.5 | 55.6 | 53.8 |
| Fresh Shallow Valley in Electris Region: ESP_033147_1350 ESP_033226_1350 (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 | -44.4 | 168. | -5.1 | 22.67 | 60.5 | 60.3 |
| Small Crater: ESP_032935_2290 ESP_033001_2290 (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 | 48.57 | 183. | 7.56 | -7.53 | 54.5 | 54.6 |
| Western Rim of Well-Preserved Impact Crater in Tyrrhena Terra: ESP_033189_1615 ESP_042011_1615 (Interval in Earth days: 688) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.5 | 98.4 | -7.3 | 8.201 | 44.6 | 44.5 |
| Possible Future Landing Site in Nili Fossae: ESP_033084_2020 ESP_033295_2020 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.58 | 78.5 | 13.0 | 2.611 | 37.5 | 38.0 |
| Fresh 2-Kilometer Diameter Impact Crater: ESP_033212_1455 ESP_041032_1455 (Interval in Earth days: 609) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 192. | -0.6 | -19.5 | 54.0 | 41.2 |
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