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.
| Strike Slip Faults in Amazonis Planitia: ESP_017045_2015 ESP_018113_2015 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.26 | 204. | -6.1 | 8.022 | 42.8 | 44.3 |
| Possible Phyllosilicate-Rich Terrain: ESP_016918_2030 ESP_017986_2030 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.68 | 71.0 | -0.6 | 12.29 | 41.6 | 43.2 |
| East Rim of Well-Preserved Crater on Rim of Larger Crater: ESP_016971_1610 ESP_017683_1610 (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 | -18.5 | 69.1 | -0.5 | 8.387 | 61.8 | 65.0 |
| Possible Chlorites and Prehnite in Northern Plains Crater: ESP_016933_2310 ESP_017210_2310 (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 | 50.48 | 16.5 | 4.76 | -14.3 | 43.8 | 44.8 |
| Persbo Crater Ejecta Covered by Lava Flows: ESP_017060_1890 ESP_017205_1890 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.912 | 156. | -8.7 | 5.039 | 47.2 | 46.8 |
| Light-Toned Mounds in Acidalia Planitia: ESP_017132_2250 ESP_017633_2250 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.43 | 345. | -6.6 | 5.659 | 42.7 | 41.6 |
| Enigmatic Pits in Southern Elysium Planitia: ESP_017284_1790 ESP_017429_1790 (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 | -1.07 | 160. | 5.24 | 19.21 | 52.3 | 52.0 |
| Nili Patera: ESP_016905_1890 ESP_035181_1890 (Interval in Earth days: 1424) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.910 | 67.6 | 0 | 17.66 | 45.7 | 47.4 |
| Thermally Distinct Crater in Arcadia Dorsa: ESP_017097_2340 ESP_017532_2340 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.62 | 218. | 3.64 | 24.24 | 44.5 | 42.0 |
| Central Structure and Layered Bedrock in 25-Kilometer Diameter Crater: ESP_017002_1535 ESP_017147_1535 (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 | -26.0 | 303. | -3.1 | 10.15 | 67.4 | 67.7 |
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