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.
| 30-Meter Diameter Pit Near Kasei Valles : ESP_044879_1955 ESP_051327_1955 (Interval in Earth days: 502) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.46 | 277. | 3.25 | -25.6 | 44.1 | 38.6 |
| Floor of Ius Chasma : ESP_044668_1720 ESP_045301_1720 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.73 | 279. | 0 | 16.27 | 56.1 | 53.4 |
| North Polar Dunes : ESP_044851_2580 ESP_044376_2580 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.78 | 307. | -3.1 | 10.62 | 57.1 | 54.5 |
| Exposure of North Polar Layered Deposits : ESP_044690_2595 ESP_044993_2595 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.26 | 17.9 | 1.40 | 17.24 | 56.9 | 57.9 |
| Central Peak of Impact Crater North of Hellas Planitia : ESP_044952_1555 ESP_062833_1555 (Interval in Earth days: 1393) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.1 | 90.0 | -6.3 | 7.712 | 66.7 | 67.7 |
| Linear Ridge Features and Possible Mounds in Lyot Crater : ESP_044967_2300 ESP_045165_2300 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.48 | 29.5 | 6.01 | -25.0 | 43.3 | 47.5 |
| Northwestern Discontinuous Ejecta and Rays of Gratteri Crater : ESP_044737_1625 ESP_044394_1625 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.5 | 199. | -24. | 11.61 | 64.0 | 62.2 |
| Depression with Layers in Nilosyrtis Mensae : ESP_044689_2305 ESP_045256_2305 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.91 | 59.3 | -4.7 | 15.20 | 42.9 | 44.8 |
| 80-Meter Crater on North Polar Layered Deposits: ESP_044862_2635 ESP_045034_2635 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.46 | 346. | 7.96 | -8.18 | 60.5 | 62.4 |
| Double Layer Ejecta Blanket of Young Crater : ESP_044886_2135 ESP_045229_2135 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.19 | 84.0 | -1.2 | -24.7 | 41.1 | 44.8 |
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