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.
| Fresh 3-Kilometer Crater in Tyrrhena Terra: ESP_026253_1680 ESP_027387_1680 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 97.7 | -8.2 | 17.03 | 59.5 | 59.1 |
| Proximal Region of Athabasca Valles: ESP_026554_1900 ESP_019829_1900 (Interval in Earth days: 524) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.961 | 157. | -5.2 | 1.324 | 47.9 | 53.4 |
| Cratered Cones in Cydonia Region: ESP_026204_2175 ESP_034762_2175 (Interval in Earth days: 667) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.24 | 348. | 1.69 | -26.7 | 40.0 | 43.5 |
| Syrtis Major Terrain Sample: ESP_026280_1975 ESP_027902_1975 (Interval in Earth days: 126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.50 | 76.7 | -5.6 | 6.391 | 44.0 | 47.8 |
| Central Peak of Crater in Syrtis Major: ESP_026386_1825 ESP_027586_1825 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.280 | 64.8 | -6.7 | 3.498 | 51.4 | 52.3 |
| Layered Deposits in Gale Crater: ESP_026291_1750 ESP_086661_1750 (Interval in Earth days: 4703) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.87 | 138. | 5.74 | 27.78 | 54.3 | 44.6 |
| Southern Ladon Basin near the Mouth of Ladon Valles: ESP_026139_1600 ESP_027616_1600 (Interval in Earth days: 115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.8 | 329. | 5.17 | -12.8 | 63.6 | 65.3 |
| How Did Valles Marineris Form?: ESP_025415_1675 ESP_026259_1675 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.3 | 294. | 0 | -17.9 | 53.1 | 60.5 |
| A Volcanic Pit Chain and Dust Avalanches : ESP_026249_2025 ESP_026750_2025 (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 | 22.26 | 202. | -7.3 | 17.82 | 42.6 | 41.8 |
| Fresh 1-Kilometer Impact Crater in Arcadia Planitia: ESP_025801_2185 ESP_025735_2185 (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 | 38.15 | 191. | -6.6 | 8.468 | 40.6 | 39.3 |
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