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.
| Unconformity in North Polar Layered Deposits: ESP_018265_2595 ESP_018160_2595 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.25 | 357. | 0.42 | -23.4 | 57.5 | 58.8 |
| Channels in Tharsis Region: ESP_018349_2005 ESP_019338_2005 (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 | 20.50 | 241. | 7.35 | -7.99 | 45.2 | 50.8 |
| Layered Terrain in Aeolis and Zephyria Regions: ESP_018392_1740 ESP_018814_1740 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.89 | 150. | 6.24 | -8.79 | 57.3 | 57.9 |
| Flank and Summit of Low Shield Volcano East of Jovis Tholus: ESP_018283_1980 ESP_019272_1980 (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 | 17.89 | 243. | 8.11 | -7.55 | 45.8 | 50.6 |
| 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 |
| 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_018387_2600 ESP_026576_2600 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.99 | 270. | -8.4 | -24.5 | 59.2 | 58.2 |
| 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 |
| 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 |
| Pitted Terrain North of Hrad Vallis: ESP_018168_2160 ESP_019012_2160 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.59 | 141. | -3.2 | -24.7 | 43.1 | 50.1 |
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