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.
| Ridge in Eastern Candor Chasma: ESP_065819_1735 ESP_065885_1735 (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 | -6.66 | 291. | -3.2 | -17.7 | 51.2 | 51.6 |
| Aram Chaos: ESP_066015_1815 ESP_065804_1815 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.686 | 339. | 12.8 | -7.98 | 52.1 | 55.4 |
| 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 |
| Cluster of Small Cones in Baetis Chaos: ESP_065977_1770 ESP_065911_1770 (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 | -2.86 | 299. | -7.7 | 6.708 | 51.7 | 51.3 |
| 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 |
| 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 |
| South Polar Layered Deposits: ESP_066063_0940 ESP_066062_0940 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -86.0 | 161. | 0.05 | 20.37 | 64.9 | 63.1 |
| 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 |
| South Polar Cap Vertical Change Monitoring: ESP_065909_0930 ESP_065989_0930 (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 | -86.7 | 16.2 | 23.3 | 8.954 | 63.8 | 64.7 |
| Layering in Arabia Terra: ESP_065922_1850 ESP_065988_1850 (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 | 5.104 | 357. | 7.70 | -6.41 | 55.1 | 55.5 |
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