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.
| Stratigraphy of Rocks in Claritas Fossae Region: ESP_012995_1530 ESP_030902_1530 (Interval in Earth days: 1395) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 258. | -7.1 | 4.769 | 43.5 | 37.3 |
| Bright Gully Deposits in Western Hale Crater: ESP_013230_1445 ESP_014074_1445 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.0 | 322. | 8.51 | -20.1 | 39.3 | 37.8 |
| Possible Fan Delta: ESP_013531_2140 ESP_022036_2140 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.87 | 17.5 | -8.5 | 21.35 | 68.7 | 68.8 |
| Light-Toned Outcrop in Hummock of Iani Chaos: ESP_013717_1790 ESP_013862_1790 (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 | -1.05 | 342. | 5.13 | 18.19 | 42.1 | 39.5 |
| Wrinkle Ridge in Lunae Palus: ESP_014022_1950 ESP_014167_1950 (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 | 14.94 | 294. | -7.9 | 7.828 | 48.7 | 45.9 |
| Light-Toned Outcrops Near Crater Rim in Arabia Terra: ESP_014165_1985 ESP_022314_1985 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.07 | 349. | 2.28 | 28.31 | 48.4 | 53.8 |
| Well-Preserved 3 Kilometer Diameter Impact Crater: ESP_012991_1335 ESP_013624_1335 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.9 | 9.53 | 3.76 | -12.3 | 44.3 | 40.8 |
| Exposure of Layered Sequence in Terby Crater: ESP_013160_1530 ESP_074031_1530 (Interval in Earth days: 4743) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 74.0 | -8.4 | 2.702 | 41.5 | 52.0 |
| North Wall of Ritchey Crater: ESP_013125_1520 ESP_013758_1520 (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 | -27.9 | 309. | 0.17 | -22.9 | 41.2 | 37.0 |
| Central Structure of a Large Impact Crater: ESP_013134_1610 ESP_021494_1610 (Interval in Earth days: 652) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.6 | 62.6 | -6.3 | 14.94 | 43.1 | 44.9 |
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