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 Part of Samara Valles System : ESP_047145_1660 ESP_047567_1660 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.7 | 337. | -5.2 | -25.7 | 51.1 | 50.1 |
| Bright and Dark Fans on Patterned Ground : ESP_047281_0950 ESP_055957_0950 (Interval in Earth days: 676) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.0 | 259. | 3.28 | 14.52 | 76.3 | 78.0 |
| Scarp Near Atlantis Chaos : ESP_047375_1450 ESP_048166_1450 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.6 | 181. | -5.4 | 20.38 | 51.2 | 38.5 |
| Curved Channel along Lava Flow Margin in Solis Planum : ESP_047319_1640 ESP_065477_1640 (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 | -15.9 | 266. | 3.82 | -7.46 | 49.3 | 51.9 |
| Candidate Recent Impact Site : ESP_047004_2110 ESP_055232_2110 (Interval in Earth days: 641) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.77 | 221. | -2.3 | -17.3 | 61.5 | 56.5 |
| Intersecting Channels near Olympica Fossae: ESP_045091_2045 ESP_044326_2045 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.30 | 249. | -4.6 | 20.49 | 42.8 | 39.4 |
| A Human Bird’s Eye View of Mars: PSP_006633_2010 PSP_007556_2010 (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 | 20.99 | 74.4 | 4.70 | -20.5 | 38.8 | 42.1 |
| Possible Layering on Crater Floor in Protonilus Mensae : ESP_046931_2250 ESP_073082_2255 (Interval in Earth days: 2037) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.88 | 52.1 | 3.57 | -7.13 | 67.1 | 67.2 |
| Candidate ExoMars Landing Site in Oxia Palus : ESP_046934_1990 ESP_064182_1990 (Interval in Earth days: 1344) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.66 | 335. | -5.7 | -17.8 | 56.4 | 59.2 |
| Surface Features of Debris Apron in Deuteronilus Mensae : ESP_046787_2210 ESP_090199_2210 (Interval in Earth days: 3382) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.80 | 23.8 | 7.56 | -18.2 | 62.6 | 59.2 |
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