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.
| 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 |
| 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 |
| Aeolis Dorsa Inverted Deposits: ESP_088612_1735 ESP_088823_1735 (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 | -6.35 | 154. | -1.4 | -14.9 | 59.6 | 60.6 |
| 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 |
| 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 |
| 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 |
| Platy-Ridged Lava: ESP_088635_2000 ESP_088780_2000 (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 | 19.88 | 243. | -1.4 | 9.447 | 47.2 | 46.7 |
| Lobate Glacial Deposit in Crater: ESP_088601_2150 ESP_088825_2150 (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 | 34.85 | 90.4 | -8.8 | 26.07 | 44.8 | 42.4 |
| Channels along Hydraotes Chaos Channel: ESP_088566_1835 ESP_088711_1835 (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 | 3.377 | 329. | 3.41 | 14.35 | 53.8 | 53.2 |
| Wrinkle Ridge and Valley Network Intersection: ESP_088616_1750 ESP_088471_1750 (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 | -4.96 | 45.5 | -4.8 | -15.5 | 59.1 | 59.6 |
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