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.
| Impact Monitoring Site in Utopia Planitia: ESP_016495_2240 ESP_028666_2240 (Interval in Earth days: 949) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.65 | 96.3 | -3.2 | 7.185 | 43.5 | 58.5 |
| Possible Landing Site for MSL in Eastern Margaritifer Terra: ESP_016499_1745 ESP_016565_1745 (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 | -5.60 | 353. | -7.2 | -27.6 | 50.0 | 52.2 |
| Cerberus Fossae: ESP_016822_1865 ESP_017600_1865 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.281 | 173. | 2.06 | -11.4 | 46.2 | 50.8 |
| Discontinuous Small Channel South of Dao Vallis: ESP_016311_1420 ESP_016588_1420 (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 | -37.6 | 89.5 | 5.56 | -17.0 | 67.7 | 72.4 |
| Fresh 3-Kilometer Diameter Crater Near Hellas Planitia: ESP_016681_1575 ESP_017393_1575 (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 | -22.1 | 67.3 | -6.1 | 7.478 | 62.0 | 66.5 |
| Field of Small Volcanoes Northeast of Ascraeus Mons: ESP_016832_1885 ESP_017254_1885 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.580 | 259. | 8.08 | -10.9 | 44.8 | 48.3 |
| Very Well-Preserved 9-Kilometer Diameter Impact Crater: ESP_016490_2315 ESP_016780_2315 (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 | 51.39 | 234. | -21. | -2.88 | 48.2 | 45.3 |
| Strata Exposed in Crater Wall Near Candidate MSL Landing Site: ESP_016829_2040 ESP_019598_2040 (Interval in Earth days: 216) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.52 | 341. | -5.4 | 8.972 | 41.7 | 51.4 |
| Dissected Terrain in Arcadia Planitia: ESP_016492_2175 ESP_017125_2175 (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 | 37.02 | 178. | 1.71 | -12.6 | 41.3 | 42.2 |
| Aram Chaos: ESP_016750_1830 ESP_017172_1830 (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 | 2.769 | 339. | 3.01 | -13.3 | 47.2 | 51.0 |
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