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.
| Layered Materials on Floor of Ritchey Crater: ESP_041977_1515 ESP_042122_1515 (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 | -28.2 | 308. | -2.2 | 11.68 | 50.1 | 51.5 |
| Lobate Flow Fronts and Terraced Knobs: ESP_041985_2190 ESP_042275_2190 (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 | 38.47 | 80.4 | 10.2 | 28.86 | 45.9 | 42.1 |
| Branching Radial Ridges within Shallow-Floored Crater: ESP_041921_1530 ESP_042066_1530 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.5 | 37.9 | -7.0 | 7.19 | 48.6 | 49.9 |
| Hydrated Materials within Orson Welles Crater: ESP_041924_1790 ESP_052130_1790 (Interval in Earth days: 795) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.97 | 313. | -19. | 7.429 | 39.3 | 47.1 |
| Clay-Rich Terrain in Oxia Planum: A Proposed ExoMars Landing Site: ESP_039154_1985 ESP_065448_1985 (Interval in Earth days: 2049) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.27 | 335. | -1.2 | -20.7 | 63.6 | 66.4 |
| Triple Crater: ESP_041350_1455 ESP_049987_1450 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.4 | 148. | 6.43 | -12.8 | 43.7 | 40.2 |
| Possible Crater in South Polar Layered Deposits: ESP_041150_0920 ESP_041046_0920 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.7 | 240. | 20.0 | 6.466 | 80.0 | 79.8 |
| Layered Crater Wall in Northwest Hellas Planitia: ESP_041116_1470 ESP_041393_1470 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.6 | 56.9 | -0.3 | -23.1 | 40.2 | 45.4 |
| Dark Capped Sinuous Ridges Aligned Radially around Basin: ESP_041437_1365 ESP_041358_1365 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.3 | 292. | 22.4 | -4.33 | 49.8 | 50.2 |
| Line of Mounds East of Chryse Planitia: ESP_041145_2125 ESP_042002_2125 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.23 | 336. | 3.48 | 17.97 | 51.3 | 41.9 |
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