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.
| Sinuous Ridge in Dark Lava Flow in Western Elysium Planitia: PSP_006723_1865 PSP_007013_1865 (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 | 6.196 | 140. | -7.6 | 15.48 | 37.8 | 37.9 |
| Scarp Likely Exposing Polar Layered Deposits in Area Not Well Observed: PSP_005774_0915 ESP_023125_0915 (Interval in Earth days: 1352) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.2 | 212. | 12.6 | 21.16 | 79.7 | 73.9 |
| 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 |
| Lobate Crater Ejecta: PSP_005867_1330 ESP_011431_1330 (Interval in Earth days: 434) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.4 | 118. | 0 | 14.15 | 48.3 | 67.4 |
| Streamlined Hills in the Western Charitum Montes: PSP_006902_1275 ESP_011398_1275 (Interval in Earth days: 350) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -52.1 | 301. | -7.0 | 7.062 | 70.2 | 70.9 |
| Light-Toned Layering along Plains Adjacent to Melas Chasma: PSP_005030_1685 ESP_012427_1685 (Interval in Earth days: 576) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.2 | 284. | 3.48 | -15.1 | 35.7 | 53.6 |
| Mawrth Vallis Phillosilicate Layers: PSP_005819_2050 PSP_006742_2050 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.68 | 339. | 3.35 | -7.74 | 46.6 | 40.7 |
| Basal Exposure of South Polar Layered Deposits: PSP_005089_1040 PSP_005313_1040 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -75.8 | 131. | -6.9 | 7.077 | 60.1 | 61.9 |
| Seasonal Monitoring: PSP_005340_0930 PSP_005523_0930 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.0 | 170. | 0.24 | 20.31 | 72.8 | 73.3 |
| Fresh Crater: PSP_005517_2240 PSP_005807_2240 (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 | 43.80 | 301. | -0.2 | 20.25 | 65.1 | 59.8 |
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