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.
| Noachis Terra Sample: ESP_016182_1560 ESP_016815_1560 (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 | -23.5 | 9.41 | 6.53 | -7.78 | 56.2 | 64.3 |
| Layers in Trough Floor and Scarp of Western Bench of Terby Crater: ESP_016206_1525 ESP_016351_1525 (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 | -27.4 | 74.5 | 8.70 | 23.26 | 59.0 | 59.9 |
| Lobate Landform North of Reull Vallis: ESP_016047_1410 ESP_020293_1410 (Interval in Earth days: 331) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.6 | 97.2 | 4.47 | -12.9 | 64.7 | 63.9 |
| Possible Clays and Chlorides Near Columbus Crater: ESP_016017_1495 ESP_016162_1495 (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 | -29.9 | 196. | -6.9 | 8.162 | 58.9 | 60.1 |
| Mantled Terrain: ESP_016135_1450 ESP_016491_1450 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.6 | 214. | -3.4 | 6.745 | 63.6 | 67.7 |
| Stranded Lobe of Material with Associated Ridge on Valley Floor: ESP_016238_2180 ESP_017161_2180 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.54 | 273. | -3.4 | 6.789 | 42.5 | 40.5 |
| Gullies: ESP_016213_2315 ESP_016714_2315 (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 | 51.36 | 234. | -6.2 | 10.38 | 48.6 | 44.5 |
| Drainage Off a Large Terrace Pond in Southern Mojave Crater: ESP_016223_1870 ESP_016368_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 | 7.099 | 327. | -2.6 | 13.92 | 42.0 | 41.8 |
| Traverse Across Massif and Derbris Apron: ESP_016277_2300 ESP_016132_2300 (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 | 49.72 | 285. | 8.51 | -1.20 | 46.3 | 48.0 |
| Well-Preserved 4-Kilometer Diameter Impact Crater: ESP_015916_1640 ESP_019463_1640 (Interval in Earth days: 277) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.7 | 71.2 | -1.4 | 15.52 | 48.5 | 59.3 |
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