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.
| Gullied Crater Wall: ESP_016191_1415 ESP_026951_1415 (Interval in Earth days: 838) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.1 | 125. | 6.43 | -7.63 | 66.4 | 79.4 |
| Crater Rim Gullies Filled with Small Dunes: ESP_015934_2165 ESP_037243_2165 (Interval in Earth days: 1660) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.09 | 292. | 1.58 | -16.4 | 42.8 | 56.6 |
| Juventae Region Mound and Possible Sulfate-Rich Terrain: ESP_015934_1760 ESP_016646_1760 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.74 | 298. | 0 | 21.43 | 42.9 | 48.4 |
| Athabasca Valles: ESP_016071_1890 ESP_024708_1890 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.934 | 155. | 7.83 | -16.8 | 39.6 | 38.8 |
| 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 |
| Crater with Rampart-Like Ejecta Exposed in Cross Section: ESP_016080_1745 ESP_025574_1745 (Interval in Earth days: 740) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.30 | 272. | 0 | 11.85 | 45.1 | 49.7 |
| 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 |
| Western Iani Chaos: ESP_016183_1770 ESP_016816_1770 (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 | -3.01 | 340. | -5.7 | -19.8 | 45.6 | 52.3 |
| 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 |
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