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.
| Unnamed, Well-Preserved Crater South of Hypanis Valles: PSP_009393_1890 PSP_010105_1890 (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 | 8.973 | 313. | -3.9 | 13.87 | 51.3 | 51.3 |
| Dark Spot Near Olmpus Mons Volcano: PSP_009502_1980 ESP_015950_1980 (Interval in Earth days: 503) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.62 | 216. | -2.0 | 26.27 | 48.1 | 36.5 |
| Water Bearing Minerals in Noctis Labyrinthus: PSP_009474_1705 PSP_010107_1705 (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 | -9.28 | 263. | -0.3 | -20.5 | 60.9 | 61.8 |
| Contact between Differing Mineralogies in West Candor Chasma: PSP_008814_1740 ESP_016317_1740 (Interval in Earth days: 584) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.10 | 283. | -3.0 | -21.3 | 58.0 | 49.5 |
| Lava Flow Margin in Amazonis Planitia: PSP_008804_2055 PSP_009226_2055 (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 | 25.51 | 192. | 6.80 | -18.1 | 43.1 | 46.4 |
| Hellas Planitia: PSP_008269_1395 ESP_017631_1395 (Interval in Earth days: 730) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.1 | 52.1 | -7.6 | 4.219 | 78.8 | 80.7 |
| Rayed Crater: PSP_009205_1665 PSP_009917_1665 (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 | -13.4 | 48.1 | 4.78 | 20.94 | 63.0 | 61.5 |
| Small Shield in Syria Planum: PSP_008894_1685 PSP_009962_1685 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.2 | 260. | -11. | 6.842 | 62.0 | 61.2 |
| Ganges Catena Pit Crater Chain Cut by Wrinkle Ridge: PSP_008326_1775 PSP_008827_1775 (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 | -2.33 | 289. | 5.91 | -12.9 | 52.9 | 56.5 |
| Coprates Chasma Wall: PSP_009156_1660 ESP_016303_1660 (Interval in Earth days: 557) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.1 | 306. | -3.3 | -16.2 | 63.9 | 53.3 |
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