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.
| Future Mars Landing Site in Acidalia Mensa: ESP_018161_2270 ESP_018227_2270 (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 | 46.68 | 331. | -1.6 | -15.5 | 43.8 | 45.4 |
| Future Mars Landing Site in Antoniadi Crater: ESP_018105_2045 ESP_018250_2045 (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 | 24.05 | 63.0 | -0.2 | 13.32 | 44.2 | 43.5 |
| Fault Scarp South of Arsia Mons: ESP_017769_1685 ESP_017914_1685 (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 | -11.6 | 241. | -9.1 | 6.675 | 61.5 | 60.8 |
| Exposure of Polar Layered Deposits: ESP_018096_2710 ESP_018071_2690 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.99 | 190. | -17. | -17.5 | 64.8 | 64.3 |
| Volcanic Rootless Constructs in the Western Tartarus Colles: ESP_017956_2065 ESP_018668_2065 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.37 | 171. | -9.0 | 6.491 | 44.1 | 45.2 |
| Possible Inverted Terrain in Parana Valles Region: ESP_017831_1570 ESP_018820_1570 (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 | -22.6 | 348. | 8.41 | -6.13 | 68.1 | 67.3 |
| Valley-Crater Intersection with Exposed Layers: ESP_018055_2120 ESP_018899_2120 (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 | 31.60 | 346. | 3.16 | -20.2 | 42.5 | 48.6 |
| Small Rayed Crater in Elysium Planitia: ESP_017785_1975 ESP_018418_1975 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.20 | 160. | 5.75 | -15.8 | 45.1 | 48.3 |
| Exposure of Polar Layered Deposits: ESP_017937_2680 ESP_018162_2680 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.13 | 304. | -19. | -25.9 | 63.3 | 64.3 |
| Sample Solis Planum: ESP_017860_1590 ESP_018005_1590 (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 | -21.0 | 278. | -6.4 | 8.741 | 67.9 | 67.1 |
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