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.
| Channel in Hellas Planitia : ESP_057928_1420 ESP_058429_1420 (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 | -37.7 | 83.9 | -4.6 | 8.373 | 34.1 | 36.1 |
| Impact Crater : ESP_058133_1175 ESP_058212_1175 (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 | -62.2 | 252. | -4.1 | 13.22 | 50.1 | 50.1 |
| Candidate Landing Site for 2020 Mission in Northeast Syrtis Major Region : ESP_057928_1980 ESP_058073_1980 (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 | 17.88 | 77.2 | -10. | 13.69 | 50.5 | 47.3 |
| Terrain Sample Near Crater : ESP_057996_1955 ESP_058207_1955 (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 | 15.32 | 20.8 | 1.07 | -13.0 | 47.1 | 45.3 |
| Pitted Mounds in Aurorae Chaos : ESP_058196_1700 ESP_057774_1700 (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 | -10.0 | 323. | 2.01 | -6.81 | 31.1 | 35.5 |
| Crater Partially Buried by Ejecta from Yuty Crater: ESP_058143_2020 ESP_058855_2020 (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 | 21.98 | 325. | 7.78 | -1.45 | 49.8 | 41.6 |
| Lava-Yardang Contacts : ESP_058110_1840 ESP_058756_1840 (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 | 3.839 | 149. | 4.99 | 17.09 | 37.9 | 31.5 |
| Gusev Crater Mesas : ESP_058096_1645 ESP_058030_1645 (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 | -15.1 | 175. | -12. | 14.44 | 31.7 | 30.0 |
| Dissected Fan or Delta in Terby Crater : ESP_058192_1510 ESP_059405_1510 (Interval in Earth days: 95) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.6 | 75.2 | -4.3 | 8.821 | 31.6 | 44.4 |
| Ancient Bedforms on Gordii Dorsum : ESP_058055_1895 ESP_058767_1895 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.255 | 210. | 3.71 | -10.2 | 42.0 | 35.8 |
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