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.
| Apron of Material in Columbus Crater: PSP_010492_1510 ESP_045278_1510 (Interval in Earth days: 2710) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.8 | 194. | -5.8 | -28.5 | 69.7 | 69.7 |
| Shalbatana Vallis: PSP_010461_1845 ESP_016619_1845 (Interval in Earth days: 480) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.397 | 315. | 0 | 0 | 54.7 | 45.8 |
| Crater in Icaria Fossae Region with Intersecting Graben: ESP_011440_1335 ESP_011941_1335 (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 | -45.9 | 234. | -5.1 | 15.24 | 68.4 | 59.6 |
| Distributary Channel South of Ascraeus Mons: PSP_010872_1865 ESP_011373_1865 (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 | 6.197 | 254. | -2.2 | 20.12 | 55.7 | 55.8 |
| Streamlined Landforms on Terraces of Ritchey Crater: PSP_010646_1510 ESP_016092_1510 (Interval in Earth days: 424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.5 | 308. | 7.57 | -9.18 | 67.6 | 59.1 |
| Large Clay and Chloride Exposure in Southeast Sirenum Fossae Region: PSP_010900_1405 ESP_016201_1405 (Interval in Earth days: 413) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 216. | -5.2 | -28.4 | 71.9 | 69.5 |
| Central Peak of Gale Crater: PSP_010428_1745 ESP_016085_1745 (Interval in Earth days: 440) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.40 | 137. | 4.52 | -23.3 | 57.8 | 46.9 |
| Cone at the Source of Athabasca Valles: PSP_010770_1905 ESP_011403_1905 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.15 | 157. | 16.7 | -7.00 | 53.1 | 58.4 |
| Possible MSL Landing Site in Gale Crater: ESP_011417_1755 ESP_011562_1755 (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 | -4.44 | 137. | -15. | 1.284 | 58.8 | 57.4 |
| The North Pole of Mars: PSP_010545_2700 PSP_010586_2700 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 89.98 | -154 | -25. | -25.6 | 76.8 | 77.4 |
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