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.
| Long Section of Exposed Stratigraphy in Eastern Candor Chasma: ESP_088607_1725 ESP_088462_1725 (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 | -7.17 | 291. | 0.37 | -10.5 | 60.0 | 60.6 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_088658_1990 ESP_088724_1990 (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 | 19.01 | 335. | 2.38 | -19.7 | 47.3 | 49.3 |
| Dune Monitoring near Utopia Rupes: ESP_088746_2270 ESP_089036_2270 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.72 | 88.9 | -3.2 | 12.36 | 45.4 | 45.6 |
| Canyon Walls in Coprates Chasma: ESP_088646_1655 ESP_088857_1655 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 306. | 4.01 | -9.22 | 64.2 | 64.9 |
| Layering in Lucus Planum: ESP_088769_1730 ESP_088980_1730 (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 | -6.74 | 187. | 5.48 | -6.90 | 59.5 | 60.3 |
| Crater Exposing Structure of Glacial Fill inside Baphyras Catena: ESP_088436_2190 ESP_088647_2190 (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 | 38.53 | 275. | -8.7 | -18.9 | 44.2 | 45.8 |
| Alluvial Fan and Light-Toned Deposits in Coprates Catena Trough: ESP_088409_1655 ESP_088119_1655 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.2 | 297. | 5.41 | -13.7 | 63.9 | 64.4 |
| North Polar Layered Deposits Structural Geology in Icy Layers: ESP_088653_2625 ESP_088693_2625 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.34 | 81.4 | 8.18 | -8.30 | 58.5 | 59.6 |
| Constraining Potential Kaolinite-Rich Deposits in Syrtis Major Planum: ESP_088694_2010 ESP_088839_2010 (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 | 20.91 | 72.9 | -8.2 | 2.656 | 47.6 | 47.1 |
| North Polar Residual Cap Topography: ESP_088751_2685 ESP_089016_2685 (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 | 88.39 | 276. | -17. | -26.2 | 64.2 | 66.2 |
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