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.
| Excellent Exposure of Layered Mound in Terby Crater: ESP_013872_1520 ESP_014017_1520 (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 | -27.5 | 74.3 | 1.04 | 15.03 | 34.6 | 33.2 |
| 3 Kilometer Diameter Crater on Edge of South Polar Layered Deposits: ESP_013344_0990 ESP_013463_0990 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -80.7 | 112. | -6.3 | -22.2 | 60.8 | 62.4 |
| Enigmatic Crater Fill: ESP_013055_1010 ESP_012818_1010 (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 | -78.8 | 68.2 | 20.0 | -4.42 | 58.4 | 61.9 |
| Terraced Double Crater in Margaritifer Sinus: ESP_014152_1505 ESP_014429_1505 (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 | -29.3 | 350. | -5.5 | -28.3 | 35.3 | 38.5 |
| Pit Crater Chain Southwest of Arsia Mons: ESP_014077_1660 ESP_058186_1660 (Interval in Earth days: 3437) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 236. | -3.3 | 8.798 | 34.6 | 29.8 |
| Fresh Central Pit Crater in Southern Highlands: ESP_012727_1540 ESP_013149_1540 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.8 | 14.6 | -3.1 | -14.1 | 46.9 | 42.2 |
| Gully and Fan in Southern Hemisphere Crater: ESP_013478_1300 ESP_021614_1300 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.5 | 34.8 | -1.1 | -21.7 | 41.9 | 48.2 |
| Light-Toned Fan-Like Features in Crater in Chryse Chaos: ESP_013256_1885 ESP_022104_1885 (Interval in Earth days: 689) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.534 | 327. | -1.4 | -13.8 | 53.6 | 52.2 |
| Gullies in Gorgonum Chaos Mesas: ESP_012747_1425 ESP_013024_1425 (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 | -37.0 | 189. | 2.86 | -20.5 | 46.1 | 44.2 |
| Layering on Floor of Noctis Labyrinthus Pit: ESP_014076_1680 ESP_021513_1680 (Interval in Earth days: 579) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 263. | -5.4 | 13.21 | 35.2 | 46.5 |
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