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 Residual Cap Topography : ESP_053511_2680 ESP_053367_2680 (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 | 88.12 | 26.1 | -21. | -29.0 | 64.2 | 64.3 |
| Crater Near Athabasca Valles : ESP_053573_1885 ESP_062145_1885 (Interval in Earth days: 668) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.272 | 154. | -2.8 | -27.2 | 48.1 | 51.3 |
| Dark Materials on Olympus Mons: ESP_012548_1980 ESP_013049_1980 (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 | 17.55 | 216. | -2.9 | 20.20 | 63.7 | 59.8 |
| Candidate ExoMars Landing Site in Oxia Palus: ESP_053184_1980 ESP_061980_1980 (Interval in Earth days: 685) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.82 | 336. | -26. | -8.44 | 45.5 | 45.3 |
| Apollinaris Patera Scarp: ESP_052900_1720 ESP_052979_1720 (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 | -8.08 | 173. | -27. | 7.918 | 57.9 | 55.8 |
| Candidate Red Dragon Landing Site in Arcadia Region: ESP_052925_2195 ESP_052859_2195 (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 | 39.35 | 203. | -4.1 | 13.14 | 39.7 | 38.1 |
| Wrinkle Ridges in West Meridiani Planum : ESP_052933_1790 ESP_052999_1790 (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 | -0.92 | 349. | -0.4 | -23.9 | 51.8 | 53.6 |
| Southern Continuous Ejecta Boundary of Zunil Crater: ESP_052821_1875 ESP_053467_1875 (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 | 7.275 | 166. | 4.03 | 28.63 | 46.6 | 45.9 |
| Exit Breach in Well-Preserved Crater: ESP_052945_2150 ESP_053222_2150 (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 | 34.79 | 17.3 | 0.22 | -25.5 | 39.3 | 42.4 |
| Candidate Red Dragon Landing Site in Arcadia Planitia : ESP_053070_2205 ESP_053202_2205 (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 | 39.92 | 202. | 8.28 | -24.2 | 39.0 | 42.3 |
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