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.
| Terrain Northeast of Pollack Crater: ESP_087786_1735 ESP_088498_1735 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.28 | 27.9 | 3.19 | -8.79 | 56.9 | 59.9 |
| North-Pole-Facing Deposit in Crater: ESP_087778_2285 ESP_088068_2285 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.34 | 240. | -10. | 2.734 | 44.8 | 43.5 |
| Isolated Dune Field in Crater Northwest of Syrtis Major Planum: ESP_087903_2050 ESP_089050_2050 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.85 | 71.6 | -17. | 0.922 | 45.3 | 47.0 |
| Layering in Heavily Cratered Lucus Planum Terrain: ESP_087820_1755 ESP_088110_1755 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.46 | 179. | 0.91 | 19.03 | 56.1 | 56.1 |
| 4-Kilometer Diameter Rayed Crater: ESP_087802_1915 ESP_088448_1915 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.13 | 309. | 0.34 | 12.37 | 48.0 | 49.1 |
| Overlapping Landslides in Crater in Margaritifer Terra: ESP_087603_1925 ESP_087880_1925 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.18 | 338. | 28.7 | 9.699 | 44.3 | 47.2 |
| Crater in Arabia Terra: ESP_087747_2200 ESP_087681_2200 (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 | 39.57 | 7.75 | -7.8 | 6.691 | 43.3 | 42.0 |
| Layered Rock Exposures in North Hellas Planitia: ESP_087745_1505 ESP_088391_1505 (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 | -29.2 | 69.5 | 8.55 | 23.00 | 71.6 | 73.2 |
| Layers in Depression Walls Revealing Structure of Crater Ice Fill: ESP_087798_2270 ESP_087719_2270 (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 | 46.69 | 54.0 | -5.1 | -28.4 | 43.9 | 46.3 |
| Athabasca Valles: ESP_087834_1895 ESP_088401_1895 (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 | 9.534 | 156. | -2.1 | -25.3 | 49.0 | 52.7 |
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