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.
| Well-Preserved Impact Crater: ESP_015905_2235 ESP_016182_2235 (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 | 42.91 | 3.36 | 3.72 | -15.9 | 45.9 | 45.8 |
| Gullied Crater Wall: ESP_015950_1395 ESP_016451_1395 (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 | -40.3 | 225. | 4.65 | 25.21 | 64.5 | 70.3 |
| Light-Toned Material on Plateau North of Aurorae Chaos: ESP_016157_1745 ESP_016790_1745 (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 | -5.39 | 330. | -6.7 | -21.1 | 46.4 | 53.5 |
| Possible Phyllosilicate-Rich Terrain: ESP_016102_2160 ESP_044044_2160 (Interval in Earth days: 2177) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.47 | 26.3 | 2.45 | 19.39 | 42.0 | 37.7 |
| Gullied Crater Wall: ESP_016191_1415 ESP_026951_1415 (Interval in Earth days: 838) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.1 | 125. | 6.43 | -7.63 | 66.4 | 79.4 |
| Light-Toned Outcrops and Unusual Ridges in Eastern Noctis Labyrinthus: ESP_015922_1720 ESP_016634_1720 (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 | -8.04 | 266. | -0.8 | 20.76 | 44.6 | 50.8 |
| Mounds on Hrad Vallis Mudflow: ESP_016256_2155 ESP_016322_2155 (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 | 35.06 | 142. | -2.8 | -19.2 | 41.7 | 43.0 |
| Layered Rocks in Ius Chasma: ESP_016225_1730 ESP_018348_1730 (Interval in Earth days: 166) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.94 | 273. | 0 | -15.1 | 47.4 | 59.4 |
| Small Valley in Eastern Hellas Planitia: ESP_016100_1385 ESP_016166_1385 (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 | -41.3 | 91.0 | 1.60 | -16.2 | 67.7 | 69.7 |
| Mantled Terrain: ESP_016135_1450 ESP_016491_1450 (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 | -34.6 | 214. | -3.4 | 6.745 | 63.6 | 67.7 |
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