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.
| A Boulder Festival in Masursky Crater: ESP_044653_1915 ESP_045286_1915 (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 | 11.12 | 327. | -6.3 | 9.174 | 46.4 | 45.4 |
| Lyot Crater Ejecta : ESP_044743_2290 ESP_044888_2290 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.48 | 26.1 | -7.7 | 6.254 | 43.1 | 42.6 |
| Channels on Alba Mons : ESP_044814_2270 ESP_045157_2270 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.47 | 246. | 6.41 | -14.1 | 41.6 | 45.4 |
| Crater with Thin Ejecta in Ismeniae Fossae Region : ESP_044769_2235 ESP_062927_2235 (Interval in Earth days: 1415) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 42.96 | 35.8 | 2.76 | -5.40 | 41.1 | 47.8 |
| Fractures and Exposed Bedrock in Lyot Crater : ESP_044756_2300 ESP_045099_2300 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.56 | 28.7 | 8.24 | -10.8 | 42.1 | 45.7 |
| Double-Terraced Crater in Arcadia Planitia : ESP_044724_2270 ESP_044869_2270 (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 | 46.75 | 183. | 5.44 | 19.31 | 41.4 | 40.8 |
| Multiple Yardang Units and Directions in Memnonia Sulci : ESP_044777_1725 ESP_086343_1725 (Interval in Earth days: 3239) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.48 | 184. | -7.6 | -17.1 | 56.3 | 45.6 |
| Candidate Landing Site for 2020 Mission in Hypanis Valles Delta : ESP_044970_1920 ESP_044693_1920 (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 | 11.92 | 314. | -7.7 | 6.83 | 46.3 | 45.1 |
| Candidate ExoMars Landing Site in Oxia Palus : ESP_044824_1985 ESP_062481_1985 (Interval in Earth days: 1376) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.08 | 336. | 23.1 | 5.898 | 41.5 | 45.8 |
| Transverse Aeolian Ridges in Scandia Cavi : ESP_044722_2570 ESP_044405_2570 (Interval in Earth days: 25) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.93 | 226. | 2.31 | 28.96 | 55.5 | 52.8 |
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