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.
| Possible Terraced Crater in Arcadia Planitia: ESP_033079_2280 ESP_033356_2280 (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 | 47.51 | 211. | 4.74 | -16.7 | 52.2 | 50.9 |
| Western Rim of Well-Preserved Impact Crater in Tyrrhena Terra: ESP_033189_1615 ESP_042011_1615 (Interval in Earth days: 688) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.5 | 98.4 | -7.3 | 8.201 | 44.6 | 44.5 |
| Ridge at Edge of Athabasca Valles: ESP_033279_1905 ESP_050804_1905 (Interval in Earth days: 1366) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.38 | 156. | 3.46 | -27.9 | 36.5 | 36.7 |
| Central Peak of Taxco Crater: ESP_033273_2010 ESP_042095_2010 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.64 | 319. | -3.3 | 11.76 | 38.3 | 37.9 |
| Hydrated Minerals along Coprates Chasma Wallrock: ESP_033010_1645 ESP_033788_1645 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.2 | 303. | 18.7 | 5.278 | 38.7 | 50.3 |
| Enigmatic Channels on the Floor of Mangala Valles: ESP_033053_1640 ESP_033264_1640 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 210. | 2.12 | -10.2 | 40.7 | 44.4 |
| Impact Crater with Central Peak: ESP_033202_1685 ESP_060393_1685 (Interval in Earth days: 2119) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.5 | 101. | 2.77 | -6.13 | 40.8 | 49.3 |
| Possible Fossil Dunes in Noachis Terra: ESP_032941_1310 ESP_033020_1310 (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 | -48.9 | 34.0 | -2.6 | 22.11 | 60.1 | 60.2 |
| Possible Lake Margin in Shalbatana Vallis: ESP_032904_1835 ESP_033537_1835 (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 | 3.523 | 316. | 5.31 | -26.9 | 34.5 | 41.8 |
| Well-Preserved Impact Crater with Steep Slopes: ESP_032975_1415 ESP_033041_1415 (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 | -38.2 | 183. | -4.1 | -24.0 | 53.1 | 55.4 |
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