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.
| Compositional Diversity in Northern Hellas Region: ESP_030092_1530 ESP_029815_1530 (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 | -26.7 | 55.2 | -12. | 17.29 | 48.7 | 49.8 |
| Deposits Containing Gypsum along Melas Chasma Floor: ESP_030044_1710 ESP_030255_1710 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.85 | 282. | -0.7 | -15.6 | 50.7 | 50.2 |
| Gullied Niquero Crater: ESP_030021_1410 ESP_030443_1410 (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 | -38.7 | 193. | 4.97 | -16.9 | 49.4 | 45.0 |
| Gullies in Southern Mid-Latitude Crater: ESP_030016_1415 ESP_031229_1415 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.9 | 331. | -5.4 | 14.22 | 50.2 | 34.8 |
| More Coverage of Distorted Layer in Noctus Labyrinthus: ESP_030071_1720 ESP_030216_1720 (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 | -8.10 | 265. | -9.3 | 1.688 | 51.3 | 49.4 |
| Light-Toned Gully Deposits in Hale Crater: ESP_030003_1440 ESP_030214_1440 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.4 | 324. | 5.96 | -8.14 | 49.1 | 47.1 |
| Streamlined Form in Athabasca Valles: ESP_030009_1895 ESP_040176_1895 (Interval in Earth days: 793) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.475 | 156. | -1.3 | -16.8 | 57.5 | 49.5 |
| Cross Section of Hummocks in Atlantis Chaos: ESP_030061_1450 ESP_030351_1450 (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 | -34.8 | 181. | 3.29 | 22.25 | 48.3 | 42.7 |
| Well-Preserved Crater Is Southern Highlands: ESP_030111_1365 ESP_030612_1365 (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 | -43.2 | 258. | -6.5 | 7.553 | 50.0 | 41.9 |
| A Crater Exposing Diverse Compositions: ESP_030079_1550 ESP_030290_1550 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.5 | 48.9 | -1.5 | -14.9 | 48.1 | 46.5 |
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