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.
| Look For Unconformity at Base of Interior Layered Deposits: PSP_006519_1730 PSP_007020_1730 (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 | -6.74 | 311. | 0 | 9.783 | 37.5 | 42.3 |
| Fresh Unnamed Crater with Ponded Materials and Gullies: PSP_005985_1455 ESP_013817_1455 (Interval in Earth days: 611) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.0 | 134. | 1.73 | 24.54 | 42.1 | 33.9 |
| Gorgonum Chaos: PSP_006906_1425 ESP_016004_1425 (Interval in Earth days: 709) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 188. | 1.20 | 29.59 | 58.9 | 61.5 |
| Impact Near the Summit of Elysium Mons: PSP_005892_2050 ESP_085342_2050 (Interval in Earth days: 6191) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.62 | 146. | -5.2 | 7.014 | 46.2 | 45.8 |
| Syrtis Major Hydrated Crater Floor and Megabreccia in Central Pit: PSP_005842_1970 ESP_011538_1970 (Interval in Earth days: 444) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.03 | 71.8 | 6.01 | -18.2 | 41.4 | 61.2 |
| Sinuous Ridge in Argyre Basin: PSP_006730_1235 PSP_007007_1235 (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 | -56.1 | 316. | 7.79 | -14.4 | 69.5 | 75.4 |
| Light-Toned Layered Rock Outcrop in Ladon Vallis: PSP_006637_1590 ESP_023383_1590 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.8 | 330. | 7.10 | 20.68 | 44.1 | 31.2 |
| Complex Banded Terrain of Floor of Hellas Basin: PSP_006278_1410 PSP_010563_1410 (Interval in Earth days: 334) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.7 | 55.4 | 0 | 13.47 | 49.7 | 73.5 |
| Layered Sediments in Tithonium Chasma: PSP_005281_1750 PSP_005703_1750 (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 | -4.92 | 270. | 10.9 | -5.09 | 35.2 | 34.1 |
| Reull Vallis and Valley Cut through Crater: PSP_006777_1405 PSP_006922_1405 (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 | -39.3 | 111. | -3.0 | 7.022 | 58.5 | 60.4 |
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