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.
| Lobate Flow Features East of Hellas Region: ESP_029035_1455 ESP_029457_1455 (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 | -34.3 | 113. | -7.5 | -21.4 | 62.3 | 58.4 |
| The Top of Coprates Chasma: ESP_028962_1645 ESP_037111_1645 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.4 | 303. | 5.11 | -21.1 | 56.1 | 62.8 |
| 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 |
| 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 |
| 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 |
| 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 |
| Candidate Future Landing Site in Trouvelot Crater : ESP_028512_1960 ESP_027114_1960 (Interval in Earth days: 109) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.85 | 346. | -13. | 15.53 | 53.2 | 45.0 |
| Crater with Central Peak in Isidis Planitia : ESP_028297_1885 ESP_034389_1885 (Interval in Earth days: 475) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.460 | 95.5 | 0.05 | -25.9 | 51.7 | 46.9 |
| Degradation Morphologies Near Milankovic Crater : ESP_028332_2360 ESP_033857_2360 (Interval in Earth days: 430) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 55.71 | 213. | 0 | -18.5 | 58.8 | 51.6 |
| Small Tributary Leading into Ares Vallis : ESP_028420_1870 ESP_028842_1870 (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 | 7.277 | 338. | -7.7 | -18.9 | 52.9 | 55.5 |
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