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.
| Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae: ESP_018225_2275 ESP_018146_2275 (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 | 47.18 | 22.7 | 5.82 | -17.3 | 43.5 | 45.3 |
| Crater with Two Concentric Central Stuctures: ESP_018282_1640 ESP_019271_1640 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.8 | 275. | 5.65 | -11.2 | 63.6 | 61.9 |
| Channel and Depression in Northeast Syrtis Major Planum: ESP_018210_1980 ESP_034772_1980 (Interval in Earth days: 1290) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.69 | 76.8 | 4.91 | -22.5 | 45.9 | 45.4 |
| North Polar Layered Deposits: ESP_018192_2680 ESP_019048_2680 (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 | 87.96 | 177. | -17. | -10.5 | 63.7 | 70.6 |
| Cones at Edge of North Polar Layered Deposits: ESP_018334_2600 ESP_026641_2600 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.05 | 275. | -5.1 | 10.19 | 58.7 | 56.0 |
| Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater: ESP_018268_2335 ESP_033854_2335 (Interval in Earth days: 1215) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.34 | 289. | -4.9 | 20.21 | 46.1 | 47.4 |
| Exposure of North Polar Layered Deposits: ESP_018237_2720 ESP_019053_2720 (Interval in Earth days: 64) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.90 | 293. | -9.5 | -21.3 | 65.1 | 73.4 |
| Possible MSL Rover Landing Site in Gale Crater Covering North Central Mound: ESP_018287_1755 ESP_018788_1755 (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 | -4.58 | 137. | -0.4 | 23.35 | 57.0 | 54.9 |
| Cones at Edge of North Polar Layered Deposits: ESP_018241_2595 ESP_027063_2595 (Interval in Earth days: 688) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.12 | 293. | -0.4 | -20.8 | 57.4 | 58.6 |
| Well-Preserved 5-Kilometer Diameter Impact Crater: ESP_018478_2150 ESP_018979_2150 (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 | 34.78 | 318. | -3.5 | 13.05 | 44.5 | 46.3 |
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