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.
Crater and Landslides in CTX Image: ESP_019647_1625 ESP_020003_1625 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.3 | 89.9 | -6.6 | 7.971 | 60.6 | 57.7 |
Densest Pit and Fracture Concentrations in Mojave Crater Fill: ESP_019625_1875 ESP_028183_1875 (Interval in Earth days: 667) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.492 | 327. | -3.2 | 6.008 | 53.2 | 51.0 |
Hematite in Capri Chasma: ESP_019652_1665 ESP_020575_1665 (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 | -13.2 | 312. | -1.1 | 11.70 | 58.6 | 53.5 |
Fracture Cutting Lava Flow East of Olympus Mons: ESP_019681_1975 ESP_019747_1975 (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 | 17.41 | 235. | 11.4 | -9.56 | 51.6 | 53.8 |
Fresh 7-Kilometer Diameter Crater Within Herschel Crater: ESP_019751_1665 ESP_020028_1665 (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 | -13.5 | 128. | 10.6 | -14.9 | 57.4 | 58.2 |
Possible Future Mars Landing Site near Mawrth Vallis: ESP_019730_2055 ESP_027167_2055 (Interval in Earth days: 580) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.21 | 339. | -15. | 5.539 | 54.8 | 43.4 |
Well-Preserved Impact Crater with Central Peak: ESP_019982_1825 ESP_020404_1825 (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 | 2.461 | 301. | 2.60 | -13.5 | 54.3 | 56.3 |
North-Central Endeavour Crater: ESP_019980_1780 ESP_018912_1780 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.15 | 354. | 22.2 | -8.32 | 53.1 | 55.9 |
Well-Preserved 22-Kilometer Diameter Crater off Ascraeus Mons: ESP_019786_1980 ESP_020063_1980 (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 | 17.96 | 249. | 13.0 | -10.3 | 52.2 | 56.3 |
Syrtis Major Dune Changes: ESP_019845_2000 ESP_020135_2000 (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 | 19.82 | 79.4 | -1.1 | 29.35 | 54.0 | 53.7 |
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