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.
| 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 |
| 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 |
| Stratigraphy in Ius Chasma Region : ESP_058079_1720 ESP_058725_1720 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.95 | 278. | -4.7 | 6.876 | 33.2 | 29.8 |
| 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 |
| Possible Olivine-Rich Terrain : ESP_057902_1570 ESP_058680_1570 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.7 | 70.6 | 4.04 | -15.5 | 30.8 | 33.4 |
| Crescentic Feature on South Polar Layered Deposits : ESP_057951_0925 ESP_057831_0925 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.6 | 240. | 7.09 | 20.50 | 68.9 | 66.4 |
| Exposed Bedrock in Terrace of 44-Kilometer Diameter Crater in Margaritifer Terra : ESP_057932_1670 ESP_057866_1670 (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 | -12.9 | 331. | -4.7 | 9.629 | 32.8 | 32.4 |
| Candidate Landing Site for 2020 Mission Near Jezero Crater : ESP_058139_1985 ESP_058429_1985 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.17 | 76.9 | -8.4 | 6.967 | 47.9 | 43.3 |
| Well-Preserved Ejecta of 20-Kilometer Crater Northeast of Ascraeus Mons : ESP_058040_1995 ESP_058831_1995 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.19 | 259. | -6.3 | 14.41 | 49.8 | 39.1 |
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