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.
| Deformed Crater in Tyrrhena Terra : ESP_028311_1635 ESP_028667_1635 (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 | -16.3 | 76.8 | -4.4 | 13.76 | 60.1 | 57.2 |
| Well-Preserved Impact Crater on Alba Patera : ESP_028410_2170 ESP_028766_2170 (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 | 36.72 | 247. | -8.1 | 1.304 | 54.1 | 58.0 |
| Utopia Planitia : ESP_028284_2210 ESP_028429_2210 (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 | 40.69 | 86.6 | -5.4 | 9.803 | 53.3 | 53.9 |
| Trough South of Noctis Labyrinthus : ESP_028212_1710 ESP_051908_1710 (Interval in Earth days: 1847) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.74 | 258. | -5.3 | -28.7 | 57.2 | 52.2 |
| Star and Barchan Dune Changes : ESP_028416_1710 ESP_033519_1710 (Interval in Earth days: 398) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.74 | 89.0 | 2.64 | -25.2 | 56.2 | 45.7 |
| Ridge-Edged Polygons in Hellas Basin : ESP_028457_1425 ESP_046272_1425 (Interval in Earth days: 1389) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.3 | 54.3 | -4.8 | 6.68 | 69.6 | 64.8 |
| Complex Superposition of Fractures : ESP_028330_2240 ESP_028620_2240 (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 | 43.77 | 270. | -9.5 | 17.29 | 55.1 | 57.0 |
| Potential Future Landing Site in Eastern Terby Crater : ESP_028377_1520 ESP_028654_1520 (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 | -27.5 | 75.0 | 13.9 | -7.90 | 63.9 | 63.2 |
| Dune Migration : ESP_028389_2560 ESP_028020_2560 (Interval in Earth days: 29) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 75.96 | 86.8 | 3.99 | -13.2 | 69.5 | 65.2 |
| Double or Elongated Shield Volcano Near Ceraunius Fossae : ESP_028344_2085 ESP_028700_2085 (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 | 28.07 | 250. | -8.2 | 5.592 | 51.9 | 54.5 |
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