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.
| Layers on Northern Rim of Hellas Basin: ESP_024408_1500 ESP_031911_1500 (Interval in Earth days: 585) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.4 | 70.8 | -7.5 | 5.233 | 51.0 | 33.6 |
| Apollinaris Sulci Indurated Dunes: ESP_024483_1675 ESP_024127_1675 (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 | -12.6 | 178. | 23.0 | 6.505 | 40.2 | 37.0 |
| Libya Montes: ESP_024460_1835 ESP_024961_1835 (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 | 3.674 | 85.6 | 7.39 | 20.84 | 35.8 | 39.0 |
| Possible Kaolinite Mound Deposits on Kashira Crater Floor: ESP_024464_1525 ESP_024965_1525 (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 | -27.2 | 341. | -4.2 | 9.459 | 50.2 | 56.8 |
| Dunes: ESP_024542_1870 ESP_024608_1870 (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 | 7.077 | 6.74 | 1.72 | -21.7 | 36.4 | 38.9 |
| Rocky Outcrops Northwest of Elysium Region: ESP_024537_2080 ESP_072314_2080 (Interval in Earth days: 3723) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.64 | 140. | 2.98 | 22.18 | 39.0 | 50.8 |
| Well-Preserved 7-Kilometer Impact Crater: ESP_024406_1475 ESP_042076_1475 (Interval in Earth days: 1377) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.1 | 125. | -4.9 | 8.886 | 52.6 | 53.5 |
| Dune Source in Crater with Wind Streaks Near Valles Marineris: ESP_024584_1655 ESP_033287_1655 (Interval in Earth days: 678) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.2 | 302. | 6.04 | -6.87 | 43.7 | 43.8 |
| Proposed Site for Future Exploration at Ladon Valles: ESP_024438_1595 ESP_024860_1595 (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 | -20.1 | 329. | 0.98 | -22.2 | 45.2 | 52.8 |
| Ganges Chasma Landslide: ESP_024333_1715 ESP_025401_1715 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.34 | 315. | -6.9 | 14.61 | 38.8 | 49.6 |
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