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.
| Lobate Feature on Slope on Northwest Hellas Region Rim: ESP_023710_1425 ESP_024000_1425 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 46.4 | -0.4 | 26.27 | 44.4 | 47.4 |
| End of Trough in South Polar Residual Cap: ESP_023504_0880 ESP_023703_0880 (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 | -87.8 | 5.71 | 7.96 | 13.33 | 82.0 | 86.1 |
| Possible Exposure of Polar Layered Deposits in Area Not Well Observed: ESP_023715_0910 ESP_023756_0910 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.8 | 316. | 24.2 | 20.11 | 84.0 | 85.5 |
| Gullies with Debris Aprons: ESP_023810_1395 ESP_023955_1395 (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 | -40.4 | 196. | 0.83 | 14.61 | 48.1 | 49.7 |
| Aeolis Planum: ESP_023785_1745 ESP_067671_1745 (Interval in Earth days: 3420) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.55 | 154. | 0 | -21.5 | 32.9 | 41.2 |
| Well-Preserved Gullied Crater: ESP_023731_1405 ESP_024021_1405 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.9 | 195. | -25. | 0.887 | 47.6 | 50.6 |
| Proposed Landing Site in Jezero Crater: ESP_023524_1985 ESP_023379_1985 (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 | 18.33 | 77.5 | -0.5 | -11.8 | 41.0 | 43.2 |
| Auqakuh Vallis Bedform Changes: ESP_023696_2110 ESP_023762_2110 (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 | 30.68 | 60.5 | -7.2 | -24.5 | 47.5 | 47.9 |
| Eastern Wall of Chasma Australe along Margin of Promethei Lingula: ESP_023590_0975 ESP_032530_0975 (Interval in Earth days: 697) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.4 | 101. | 6.76 | 22.90 | 77.3 | 78.5 |
| Possible Chloride Salts in Icaria Planum: ESP_023716_1420 ESP_031918_1420 (Interval in Earth days: 639) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.5 | 242. | -1.3 | -14.5 | 44.9 | 38.4 |
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