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.
| Small Fresh Crater: ESP_031847_1690 ESP_032124_1690 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.8 | 15.8 | 2.34 | -15.9 | 32.4 | 33.3 |
| Slopes South of Large Crater in Coprates Chasma: ESP_031850_1675 ESP_032206_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 | -12.5 | 294. | -4.3 | 15.40 | 32.6 | 31.0 |
| Exposure of Polar Layered Deposits Not Observed by MGS: ESP_031920_0915 ESP_031879_0915 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.4 | 268. | 14.8 | 22.22 | 74.9 | 73.3 |
| Faulted Layered Deposits in West Candor Chasma: ESP_031824_1740 ESP_031758_1740 (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 | -5.74 | 283. | -4.6 | 18.32 | 34.4 | 33.2 |
| Crater with Debris Aprons in Tyrrhena Terra: ESP_031805_1545 ESP_031950_1545 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.2 | 84.1 | 3.68 | 21.79 | 32.2 | 31.3 |
| Valleys in Tyrrhena Terra: ESP_031817_1410 ESP_031751_1410 (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 | -38.8 | 118. | 5.17 | 22.85 | 36.9 | 35.1 |
| Eastern Valles Marineris Bedrock Stratigraphy and Falling Dunes: PSP_010277_1650 PSP_010699_1650 (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 | -14.6 | 302. | -8.0 | -24.2 | 63.3 | 63.2 |
| Sedimentary Bedrock Diversity in Terby Crater: ESP_031212_1525 ESP_031278_1525 (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 | -27.1 | 73.9 | 17.1 | -4.75 | 33.2 | 34.5 |
| Possible Preserved Impact Melt Flow on the Ejecta of Bakhuysen Crater: ESP_031201_1555 ESP_031056_1555 (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 | -24.3 | 13.8 | 17.1 | 1.41 | 33.5 | 36.1 |
| Northern Hellas Planitia Layered Bedrock: ESP_031120_1505 ESP_031898_1505 (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 | -28.9 | 67.3 | 0 | -13.4 | 35.4 | 34.8 |
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