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.
| Ancient Crust Outcrops at Nectaris Montes: ESP_084519_1650 ESP_084018_1650 (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 | -14.7 | 304. | -17. | -6.83 | 37.1 | 40.8 |
| Small Terraced Crater: ESP_084549_2150 ESP_084628_2150 (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 | 34.88 | 198. | -7.5 | 14.22 | 64.1 | 61.8 |
| Exposed Crater Wall Strata in Oxia Planum: ESP_084610_1965 ESP_085533_1965 (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 | 16.27 | 334. | -4.0 | 7.925 | 49.6 | 39.9 |
| Southeast Aeolis Dorsa Inverted Delta Trunk Channel: ESP_084854_1735 ESP_084999_1735 (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 | -6.32 | 154. | -2.4 | 9.423 | 36.0 | 34.5 |
| Channels in Warrego Valles: ESP_084850_1375 ESP_092221_1375 (Interval in Earth days: 575) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.2 | 267. | 4.95 | -16.5 | 41.9 | 46.7 |
| Gully with Possible Bright Deposit: ESP_084576_1385 ESP_085222_1385 (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 | -41.2 | 190. | -4.9 | 8.917 | 39.9 | 45.6 |
| Hill on South Polar Layered Deposits: ESP_084887_0900 ESP_084374_0900 (Interval in Earth days: 40) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.7 | 35.5 | 29.4 | 29.44 | 75.3 | 68.6 |
| Ring-Mound Landforms on Schiaparelli Crater Floor: ESP_084635_1760 ESP_084859_1760 (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 | -3.73 | 14.8 | -10. | 26.07 | 38.9 | 34.4 |
| Overlapping Debris Aprons within Ganges Chasma: ESP_084848_1720 ESP_085138_1720 (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 | -8.01 | 318. | -8.1 | 20.34 | 36.1 | 33.3 |
| Gullied Crater Wall: ESP_084670_1435 ESP_085593_1435 (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 | -35.9 | 142. | 2.83 | 23.40 | 37.7 | 47.0 |
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