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.
| Fractures in Chryse Planitia: ESP_027959_1990 ESP_028737_1990 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.71 | 321. | -5.3 | 7.285 | 48.9 | 53.3 |
| Fan of Overlapping Curvilinear Ridges in Saheki Crater: ESP_028021_1580 ESP_028865_1580 (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 | -21.8 | 73.2 | 6.27 | -5.89 | 63.6 | 59.3 |
| Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor: ESP_027969_1635 ESP_028325_1635 (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 | -16.2 | 54.6 | -23. | -4.61 | 62.8 | 60.0 |
| Fretted Terrain Valley in Viking 084A73 and MOC SP2-45006: ESP_027889_2140 ESP_036394_2140 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.72 | 70.1 | -2.1 | 11.65 | 47.6 | 45.5 |
| Cut Crater along Edge of Candor Chasma: ESP_027947_1745 ESP_028013_1745 (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 | -5.65 | 291. | 9.07 | -13.0 | 55.3 | 56.8 |
| IR-Distinct Crater in Utopia Planitia: ESP_027941_2295 ESP_033110_2295 (Interval in Earth days: 403) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.18 | 88.4 | -2.7 | -19.2 | 51.3 | 54.5 |
| Crater on Valles Marineris Floor: ESP_027802_1685 ESP_028501_1685 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.5 | 290. | 3.04 | -12.9 | 58.9 | 58.1 |
| Well-Preserved Crater in Margaritifer Terra: ESP_027800_1685 ESP_028789_1685 (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 | -11.2 | 345. | -7.1 | 8.055 | 59.5 | 55.6 |
| Flow Boundary in Elysium Planitia: ESP_028149_2085 ESP_028215_2085 (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 | 28.29 | 172. | 4.18 | -12.8 | 49.0 | 51.1 |
| Colorful Surface near Nili Fossae: ESP_019753_2000 ESP_019898_2000 (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 | 19.72 | 72.4 | -16. | -0.39 | 54.6 | 54.4 |
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