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.
| Flow Margin Fracturing Northwest of Elysium Mons : ESP_048932_2135 ESP_049222_2135 (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 | 33.05 | 139. | -2.6 | 22.16 | 64.2 | 59.3 |
| Possible Flow Material at Bakhuysen Crater Rim : ESP_048950_1575 ESP_049095_1575 (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 | -22.4 | 14.6 | 0.32 | 15.89 | 32.0 | 29.9 |
| Central Uplift of Crater in Tyrrhena Terra : ESP_048921_1555 ESP_049066_1555 (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 | -24.4 | 87.5 | -9.7 | 5.579 | 32.9 | 30.8 |
| Dipping Layers Near Reull Vallis : ESP_048986_1415 ESP_058151_1415 (Interval in Earth days: 714) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.3 | 113. | 3.21 | 20.49 | 33.8 | 33.2 |
| Spider Topography : ESP_048932_0970 ESP_040453_0970 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.9 | 167. | 5.54 | 20.66 | 62.6 | 65.3 |
| Isolated Secondary Crater Cluster from Resen Crater in Hesperia Planum : ESP_048973_1520 ESP_049540_1520 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.6 | 108. | -7.9 | 4.183 | 32.5 | 31.5 |
| Crater with Steep Slopes : ESP_048648_1365 ESP_048938_1365 (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 | -43.3 | 344. | -10. | 10.17 | 37.8 | 35.3 |
| Tilted Block in Subsided Region South of Orson Welles Crater : ESP_048873_1780 ESP_049651_1780 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.97 | 314. | 2.45 | 12.36 | 39.7 | 31.5 |
| Discontinuous Sinuous Ridge within Valley : ESP_048681_1435 ESP_065903_1435 (Interval in Earth days: 1342) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.0 | 160. | 6.13 | 20.21 | 34.3 | 43.0 |
| Gullies and Arcuate Ridges in Nereidum Montes : ESP_048623_1385 ESP_049124_1385 (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 | -41.2 | 307. | -23. | -8.80 | 38.3 | 35.9 |
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