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 Terrain between Aeolis and Zephyria Plana: ESP_020594_1735 ESP_020739_1735 (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 | -6.38 | 153. | -1.7 | 14.49 | 54.5 | 52.8 |
| Central Structure of Large Impact Crater: ESP_020695_1440 ESP_029398_1440 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.5 | 280. | -0.9 | 26.38 | 56.6 | 55.8 |
| Possible Carbonate-Rich Terrain in Central Stucture of Leighton Crater: ESP_020492_1830 ESP_021481_1830 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.023 | 57.7 | -3.5 | -19.7 | 55.7 | 54.9 |
| Central Peak of an Impact Crater in Promethei Terra: ESP_020846_1400 ESP_029536_1400 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.5 | 118. | 1.54 | -24.2 | 55.4 | 59.0 |
| Ridges in Meridiani Planum: ESP_020560_1835 ESP_028551_1835 (Interval in Earth days: 623) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.475 | 0.44 | 5.90 | 25.06 | 55.1 | 51.1 |
| Crater Fill Deposit: ESP_020532_1465 ESP_020677_1465 (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 | -33.1 | 50.6 | -7.0 | 7.211 | 58.6 | 55.7 |
| Material Flowing Through Gap in Crater Rim East of Hellas Planitia: ESP_020543_1345 ESP_029246_1345 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.2 | 111. | -0.3 | 25.69 | 62.1 | 61.5 |
| Fresh 3-Kilometer Diameter Rayed Crater on Preexisting Crater Terrace: ESP_020752_1500 ESP_021596_1500 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.5 | 163. | 0.50 | -27.6 | 54.5 | 45.8 |
| Terrain between Aureum and Hydaspis Chaos: ESP_020416_1805 ESP_073151_1805 (Interval in Earth days: 4109) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.240 | 333. | -6.3 | 3.415 | 55.6 | 57.2 |
| Ejecta of Very Well-Preserved Crater: ESP_020723_2235 ESP_064845_2235 (Interval in Earth days: 3438) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.26 | 225. | -4.6 | 28.28 | 72.1 | 71.8 |
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