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.
| Remnant Dissected Surface : ESP_046786_1570 ESP_046931_1570 (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 | -22.7 | 61.0 | -8.3 | 7.391 | 54.9 | 52.6 |
| Possible Layering on Crater Floor in Protonilus Mensae : ESP_046931_2250 ESP_073082_2255 (Interval in Earth days: 2037) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.88 | 52.1 | 3.57 | -7.13 | 67.1 | 67.2 |
| Monitoring Region Dubbed Ithaca : ESP_046770_0950 ESP_046769_0950 (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 | -85.1 | 180. | -6.4 | 20.15 | 86.7 | 84.5 |
| Youthful Small Crater in CTX Image: ESP_046834_1525 ESP_047691_1525 (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 | -27.1 | 190. | -5.1 | 6.348 | 55.5 | 45.3 |
| Surface Features of Debris Apron in Deuteronilus Mensae : ESP_046787_2210 ESP_090199_2210 (Interval in Earth days: 3382) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.80 | 23.8 | 7.56 | -18.2 | 62.6 | 59.2 |
| Concentric Crater Fill in Southern Mid-Latitudes : ESP_046622_1365 ESP_046688_1365 (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 | -43.1 | 219. | 6.81 | -10.9 | 63.6 | 63.9 |
| Small Dome and Barchan Dunes in Newton Crater : ESP_046649_1385 ESP_046504_1385 (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 | -41.1 | 202. | 2.56 | -11.2 | 62.5 | 65.3 |
| Classic Spider Plumes in Region Dubbed Manhattan : ESP_046641_0935 ESP_046642_0935 (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 | -86.3 | 99.0 | 8.03 | -7.68 | 88.8 | 90.5 |
| Pitted Cones in Hydraotes Chaos : ESP_046763_1785 ESP_046908_1785 (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 | -1.31 | 326. | -8.1 | 9.35 | 52.2 | 50.9 |
| East Coprates Chasma Wall Slopes : ESP_046764_1660 ESP_050812_1660 (Interval in Earth days: 315) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 300. | -8.8 | -20.4 | 53.2 | 41.3 |
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