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.
| West Arabia Region Crater with Layered Mound in THEMIS V06316014: ESP_034392_1950 ESP_035038_1950 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.84 | 10.9 | -4.4 | 18.88 | 43.0 | 44.1 |
| Pits and Channels on East Flank of Ascraeus Mons: ESP_034317_1955 ESP_034528_1955 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.15 | 257. | 8.85 | -5.48 | 41.4 | 43.6 |
| Crater in Northern Syrtis Major: ESP_034258_1955 ESP_035814_1955 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.24 | 68.7 | 2.74 | -19.7 | 41.5 | 49.3 |
| InSight Mission Candidate Landing Site: ESP_034427_1840 ESP_035851_1840 (Interval in Earth days: 111) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.830 | 136. | -6.2 | 19.3 | 47.5 | 51.5 |
| Possible Terraced Crater in Arcadia Planitia: ESP_034319_2260 ESP_034754_2260 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.67 | 198. | 3.45 | 23.42 | 42.8 | 40.0 |
| Terraced Slope in CTX Image: ESP_034231_2080 ESP_035444_2080 (Interval in Earth days: 95) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.77 | 87.2 | -26. | -8.34 | 42.5 | 43.7 |
| Candidate Future Landing Site in Trouvelot Crater: ESP_034472_1960 ESP_026336_1960 (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 | 15.89 | 347. | -13. | 4.747 | 43.8 | 44.0 |
| Meander in Central Channel in Nanedi Valles: ESP_034236_1855 ESP_035792_1855 (Interval in Earth days: 121) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.183 | 310. | 3.71 | -19.7 | 44.7 | 53.6 |
| Inner Layers of Mojave Crater Ejecta: ESP_034420_1885 ESP_034354_1885 (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 | 8.350 | 327. | -2.5 | 21.49 | 45.2 | 42.9 |
| Crater-Related Pitted Materials in 8-Kilometer Diameter Hellas Region Crater: ESP_034297_1380 ESP_034363_1380 (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 | -41.9 | 91.6 | 1.75 | -17.4 | 75.1 | 76.9 |
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