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.
| Multiple Geologic and Geomorphic Units in Contact : ESP_029151_1695 ESP_029296_1695 (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 | -10.4 | 182. | 4.21 | 20.99 | 54.6 | 52.7 |
| Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor : ESP_029103_1675 ESP_029037_1675 (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 | -12.5 | 54.0 | -1.6 | 21.19 | 55.5 | 53.9 |
| Collapse Structures South of Orson Welles Crater : ESP_028988_1775 ESP_028355_1775 (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 | -2.69 | 313. | -10. | 6.729 | 55.4 | 54.0 |
| Landform Transition from Chaos Terrain to Outflow Channel : ESP_029106_1855 ESP_034921_1855 (Interval in Earth days: 453) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.330 | 330. | -6.7 | -24.7 | 55.3 | 51.3 |
| Kasei Valles Lava Surface : ESP_029147_2015 ESP_055335_2015 (Interval in Earth days: 2041) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.36 | 287. | 5.39 | 17.42 | 57.5 | 52.4 |
| Light-Toned Fractures in Uzboi Vallis: ESP_029014_1525 ESP_038495_1525 (Interval in Earth days: 739) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.3 | 324. | 8.88 | 0.117 | 58.8 | 54.9 |
| Western Portion of Central Structure in Mazamba Crater : ESP_029134_1520 ESP_029846_1520 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 290. | -11. | 0.335 | 59.2 | 50.7 |
| Knob in Northwest Hellas Planitia : ESP_028958_1525 ESP_037753_1525 (Interval in Earth days: 686) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 55.0 | -7.6 | 19.46 | 60.4 | 60.5 |
| Possible Vent in Ceraunius Fossae : ESP_028977_2065 ESP_029122_2065 (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 | 26.26 | 249. | -7.5 | 6.811 | 58.2 | 58.6 |
| Lava-Carved Gullies in a Crater: ESP_028321_1785 ESP_037749_1785 (Interval in Earth days: 734) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.25 | 161. | -3.2 | 10.20 | 54.3 | 55.8 |
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