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.
| Putative Chlorides near Columbus Crater: ESP_017283_1490 ESP_017428_1490 (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 | -30.5 | 193. | -13. | -0.28 | 73.1 | 73.1 |
| Coprates Chasma Wall: ESP_017200_1680 ESP_017912_1680 (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 | -11.7 | 296. | -9.0 | 1.653 | 59.3 | 61.1 |
| Candidate MSL Landing Site in Northeast Syrtis Major: ESP_016931_1980 ESP_017076_1980 (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 | 17.80 | 77.0 | -4.2 | 8.612 | 43.0 | 42.6 |
| Possible Sulfates in Ius Chasma: ESP_016937_1725 ESP_018849_1725 (Interval in Earth days: 149) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.21 | 275. | 2.75 | -12.9 | 54.0 | 58.8 |
| Crater near Mawrth Vallis: ESP_017053_2060 ESP_017686_2060 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.64 | 344. | -0.4 | -23.8 | 41.5 | 45.0 |
| Fluvial Features Northwest of the Elysium Region: ESP_017285_2140 ESP_017707_2140 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.83 | 128. | 5.01 | -9.66 | 40.6 | 42.5 |
| Debris Apron Terrain in Deuteronilus Mensae: ESP_017170_2250 ESP_017671_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 | 44.66 | 28.3 | -6.2 | 5.977 | 42.6 | 41.6 |
| Diverse Lava Morphologies in Elysium Planitia: ESP_017271_1870 ESP_017416_1870 (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 | 6.820 | 155. | -6.6 | 7.712 | 48.9 | 48.5 |
| Megabreccia on Floor of Stokes Crater: ESP_016980_2360 ESP_017257_2360 (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 | 55.59 | 171. | 8.30 | -8.42 | 45.3 | 45.8 |
| Eastern Ejecta of Zumba Crater: ESP_017229_1510 ESP_017374_1510 (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 | -28.6 | 227. | -7.4 | 6.288 | 71.1 | 71.1 |
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