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.
| North Polar Crater Dune Changes: ESP_026863_2535 ESP_026876_2535 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.51 | 348. | -1.0 | 13.52 | 53.2 | 52.2 |
| Northern Plains Craters: ESP_026987_2305 ESP_027264_2305 (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 | 50.36 | 208. | 11.3 | -1.28 | 42.7 | 45.3 |
| Flow Boundary in Phlegra Region: ESP_026883_2115 ESP_027582_2115 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.15 | 172. | 1.57 | -15.1 | 41.8 | 46.4 |
| Crater Filled By Kasei Valles Flow: ESP_026826_2025 ESP_027103_2025 (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 | 22.05 | 289. | 1.09 | -19.6 | 43.4 | 46.0 |
| Hibes Montes: ESP_026659_1845 ESP_027226_1845 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.268 | 170. | 0 | 14.08 | 50.6 | 50.3 |
| Viscous Flow in Deuteronilus Mensae: ESP_026849_2235 ESP_026348_2235 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.34 | 17.3 | 11.3 | -8.75 | 40.8 | 41.6 |
| Central Peak of Ottumwa Crater: ESP_026931_2050 ESP_027709_2050 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.56 | 304. | -14. | 5.156 | 44.4 | 45.9 |
| Ridges in Meridiani Planum: ESP_026718_1825 ESP_026362_1825 (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 | 2.679 | -0.4 | 11.8 | -0.58 | 50.8 | 50.7 |
| Possible Future Landing Site in Sabrina Vallis Delta: ESP_026601_1920 ESP_034605_1920 (Interval in Earth days: 623) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.68 | 313. | 3.61 | 21.97 | 46.6 | 43.1 |
| Crater on Northern Plains: ESP_026880_2355 ESP_026959_2355 (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 | 55.32 | 253. | -20. | -1.45 | 46.5 | 45.1 |
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