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.
| Crater in Arabia Terra: ESP_068336_2245 ESP_069075_2245 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.10 | 6.10 | 4.50 | 28.14 | 54.1 | 47.6 |
| 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 |
| 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 |
| Landforms on Floor of Wahoo Crater: ESP_067902_2040 ESP_067493_2040 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.50 | 326. | 8.19 | -6.89 | 46.5 | 50.7 |
| Lobate Debris Apron on Floor of Barnard Crater: ESP_067833_1185 ESP_067688_1185 (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 | -61.0 | 60.2 | 11.4 | -14.6 | 64.7 | 63.7 |
| Complex Crater Fill and Erosion: ESP_067822_1860 ESP_067690_1860 (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 | 6.047 | 352. | -8.4 | 7.125 | 42.0 | 40.8 |
| Layered Deposits in West Candor Chasma: ESP_067785_1755 ESP_067983_1755 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.63 | 283. | -10. | -25.6 | 40.8 | 43.3 |
| Terrain Sample: ESP_067995_1650 ESP_067520_1650 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.7 | 313. | 24.1 | 7.839 | 41.1 | 38.2 |
| Candidate Braided-River Deposit in Arabia Region: ESP_068006_2175 ESP_069062_2175 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.33 | 7.09 | 11.2 | -10.6 | 52.8 | 49.2 |
| Gullies with Bright Fans in Noachis Terra: ESP_067743_1475 ESP_077265_1475 (Interval in Earth days: 742) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.1 | 351. | 3.61 | -6.16 | 46.0 | 54.6 |
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