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.
| Utopia Planitia Craters: ESP_077354_2255 ESP_077222_2255 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.31 | 73.0 | -8.2 | 8.288 | 51.4 | 51.5 |
| Glacial (Ice) or Lava Flow?: ESP_076502_2100 ESP_077333_2100 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.66 | 285. | 5.10 | 15.32 | 49.4 | 42.1 |
| Arsia Mons Southwestern Caldera Wall: ESP_077335_1700 ESP_077269_1700 (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 | -10.0 | 239. | -14. | -0.73 | 44.5 | 42.8 |
| Surface Bands on Lobate Debris Apron with High Sinuosity: ESP_077210_2140 ESP_077988_2140 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.46 | 44.2 | -7.0 | 8.687 | 46.1 | 42.1 |
| Northern Plains Flow Features: ESP_077449_2235 ESP_078438_2235 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.31 | 0.37 | -2.0 | -24.7 | 49.1 | 46.5 |
| Layers in West Melas Chasma: ESP_077109_1715 ESP_077043_1715 (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 | -8.53 | 285. | -7.5 | 6.737 | 41.0 | 39.2 |
| Glacial Erosion and Mantled Central Pit Crater: ESP_077151_2185 ESP_077362_2185 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.05 | 213. | -6.7 | 11.34 | 48.9 | 46.0 |
| Lava in Kasei Valles: ESP_077122_2025 ESP_077399_2025 (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 | 22.09 | 286. | -4.9 | 5.772 | 41.7 | 40.4 |
| Aram Chaos: ESP_077107_1820 ESP_077384_1820 (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 | 2.106 | 338. | -5.4 | 6.296 | 38.8 | 39.9 |
| Crater: ESP_077219_1455 ESP_085157_1455 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -34.1 | 167. | -6.1 | -22.1 | 55.1 | 42.9 |
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