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.
| The Oldest Sedimentary Rocks on Mars: ESP_049832_1560 ESP_049898_1560 (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 | -23.9 | 57.3 | -1.5 | -19.2 | 32.8 | 34.7 |
| Southern Canyon Wall in East Coprates Chasma: ESP_081605_1640 ESP_081671_1640 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 304. | 7.52 | -13.4 | 60.9 | 62.2 |
| Well-Preserved 15-Km Impact Crater: ESP_081590_1700 ESP_082223_1700 (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 | -9.66 | 353. | 7.67 | 22.76 | 59.3 | 56.1 |
| Isolated Dunes and Sand Patches Southeast of Syrtis Major: ESP_081600_1980 ESP_089986_1980 (Interval in Earth days: 654) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.60 | 78.4 | -13. | 8.609 | 58.3 | 52.4 |
| Light-Toned Exposures near Voeykov Crater: ESP_081685_1465 ESP_081619_1465 (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 | -33.2 | 283. | -1.0 | 17.80 | 67.2 | 66.5 |
| North Polar Scarp: ESP_081654_2595 ESP_081667_2595 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.28 | 27.7 | -5.2 | 4.363 | 79.0 | 78.6 |
| Layered Material in Idaeus Fossae Crater Wall: ESP_081565_2165 ESP_081710_2165 (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 | 36.21 | 311. | -7.5 | 7.792 | 60.4 | 61.0 |
| Group of Channels in Tyrrhena Terra: ESP_081639_1575 ESP_081784_1575 (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 | -22.3 | 97.3 | 2.87 | 23.04 | 63.2 | 60.7 |
| Shallow Raised-Rimmed Depression with Lobate Margin: ESP_081669_2165 ESP_081814_2165 (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 | 36.13 | 350. | 3.35 | 19.09 | 60.8 | 61.4 |
| Long Ridge and Phyllosilicate-Rich Terrain in Nili Fossae: ESP_081587_2020 ESP_081864_2020 (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 | 21.94 | 72.1 | -5.4 | -21.7 | 57.9 | 61.7 |
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