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.
| Floor of East Candor Chasma: ESP_034685_1730 ESP_034751_1730 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.78 | 292. | 11.1 | -13.5 | 53.9 | 56.0 |
| Change Detection in Chain of Small Pits North of Alba Patera: ESP_034699_2310 ESP_034831_2310 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.52 | 263. | -1.2 | -27.3 | 43.6 | 45.8 |
| Layered Rocks of Ophir Mensa: ESP_034738_1760 ESP_034949_1760 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.81 | 285. | -3.5 | -14.7 | 53.5 | 55.5 |
| Domoni Crater Secondaries: ESP_034845_2305 ESP_035280_2305 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.02 | 236. | -1.8 | 22.27 | 43.3 | 41.1 |
| Sinuous Ridges inside Crater in Aeolis Dorsa: ESP_034545_1740 ESP_036879_1740 (Interval in Earth days: 182) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.97 | 154. | 8.74 | -3.37 | 52.5 | 58.0 |
| Crater with Light and Dark Layers Exposed in Walls: ESP_034733_1675 ESP_035023_1675 (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 | -12.4 | 63.9 | -7.9 | 19.17 | 59.0 | 59.1 |
| Faulted Plains in Tempe Terra: ESP_034791_2245 ESP_035081_2245 (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 | 44.15 | 271. | 6.29 | 23.09 | 41.3 | 39.7 |
| Crater with Steep Slopes: ESP_034850_1895 ESP_053588_1895 (Interval in Earth days: 1460) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.227 | 105. | 7.15 | -6.01 | 46.6 | 47.9 |
| Channels on Mesa in Southern Elysium Planitia: ESP_034558_1775 ESP_052307_1775 (Interval in Earth days: 1383) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.48 | 159. | 6.18 | 26.96 | 50.8 | 47.7 |
| Transverse Aeolian Ridges in Aram Chaos: ESP_034881_1825 ESP_036437_1825 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.510 | 340. | 0.54 | 14.10 | 50.6 | 53.1 |
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