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.
| Low Thermal Inertia Mound in Terra Sabaea Bedrock Plain: ESP_066039_1605 ESP_074968_1605 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.0 | 48.7 | -2.1 | 8.696 | 44.8 | 41.0 |
| Terrain Sample: ESP_065892_1370 ESP_066024_1370 (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 | -42.7 | 102. | 7.30 | -14.7 | 45.0 | 45.3 |
| Gully Monitoring and Topography: ESP_066072_1375 ESP_065175_1375 (Interval in Earth days: 70) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.9 | 232. | -10. | 6.942 | 44.4 | 54.5 |
| Athabasca Valles Distributary: ESP_066035_1875 ESP_057978_1875 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.385 | 153. | 7.18 | -7.96 | 55.4 | 42.4 |
| Bisected Polygonal Bedrock: ESP_065918_1935 ESP_083234_1935 (Interval in Earth days: 1349) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.13 | 106. | -3.5 | 4.659 | 60.4 | 61.0 |
| Ostrov Crater Fans: ESP_065778_1530 ESP_066543_1530 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.4 | 331. | 4.24 | 27.83 | 46.0 | 36.6 |
| Possible Sulfate-Rich Terrain: ESP_065964_1720 ESP_065898_1720 (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 | -7.74 | 294. | -8.1 | 6.721 | 49.7 | 49.3 |
| Valles Marineris: ESP_066004_1745 ESP_065938_1745 (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 | -5.45 | 282. | -8.2 | 6.452 | 50.2 | 49.9 |
| Central Pit Crater with Possibly Active Slope Processes: ESP_065704_1480 ESP_065770_1480 (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 | -31.6 | 191. | 7.68 | -6.72 | 46.3 | 46.6 |
| Gully Monitoring and Topography: ESP_065837_1415 ESP_066589_1415 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.0 | 163. | 4.75 | -23.9 | 45.1 | 41.7 |
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