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.
| Layered Deposits on South Wall of West Candor Chasma: ESP_068392_1730 ESP_076832_1730 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.96 | 284. | 21.9 | 0.965 | 43.9 | 37.3 |
| Polygonal Cracks in Galilaei Crater: ESP_068377_1855 ESP_069314_1855 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.364 | 333. | 7.64 | -6.05 | 42.9 | 52.1 |
| Fresh Crater: ESP_068112_1615 ESP_068706_1615 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.1 | 4.43 | -0.2 | -8.83 | 45.6 | 54.9 |
| Rimless Crater with Gullies: ESP_068186_1445 ESP_073659_1445 (Interval in Earth days: 426) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.9 | 148. | -6.7 | 8.797 | 55.1 | 57.1 |
| Crater in Arabia Terra: ESP_068257_2180 ESP_069326_2180 (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 | 37.73 | 1.86 | 4.48 | -9.08 | 51.4 | 48.9 |
| Crater with Outlet Channel in Southern Highlands: ESP_068258_1480 ESP_073665_1480 (Interval in Earth days: 421) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -31.5 | 344. | -6.6 | 9.163 | 54.4 | 56.4 |
| Expanded Secondary Crater Cluster in Arcadia Planitia: ESP_068250_2220 ESP_069187_2220 (Interval in Earth days: 73) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.65 | 193. | -8.2 | 0.857 | 54.4 | 49.0 |
| Completely Filled Glacial Crater in Phlegra Montes: ESP_068207_2195 ESP_072480_2195 (Interval in Earth days: 332) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.12 | 284. | 7.99 | 29.27 | 52.2 | 53.5 |
| Inverted Channel East of Arabia Terra: ESP_068163_1965 ESP_069021_1965 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.13 | 49.6 | -6.4 | -20.8 | 44.3 | 48.6 |
| Streamlined Form in Kasei Valles: ESP_068326_1990 ESP_069474_1990 (Interval in Earth days: 89) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.78 | 283. | -7.8 | 6.899 | 45.0 | 48.4 |
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