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.
| Embayed Crater in Western Elysium Planitia: ESP_011720_1835 ESP_012353_1835 (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 | 3.484 | 142. | 7.82 | -9.32 | 57.5 | 58.2 |
| Eastern Half of Well-Preserved 7-Kilometer Diameter Gullied Crater: ESP_012483_1425 ESP_012338_1425 (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 | -37.2 | 198. | -5.3 | -17.7 | 50.7 | 53.8 |
| Unusual and Pristine Crater Morphology: ESP_011717_1910 ESP_012429_1910 (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 | 10.63 | 224. | -6.7 | 14.06 | 59.9 | 59.2 |
| Folded Layered Deposits: ESP_012305_1865 ESP_012371_1865 (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 | 6.390 | 11.8 | 1.20 | -19.8 | 58.6 | 60.1 |
| Grand Canyon of Gale Crater: ESP_012340_1750 ESP_012195_1750 (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 | -5.18 | 137. | 5.40 | -12.9 | 54.3 | 56.5 |
| Possible Olivine-Rich Terrain: ESP_012501_1590 ESP_092215_1590 (Interval in Earth days: 6211) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -20.8 | 64.0 | 0.76 | 27.93 | 50.0 | 43.3 |
| Contact between Wallrock and Light-Toned Rocks in Ophir Chasma: ESP_011662_1750 ESP_011807_1750 (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 | -4.76 | 287. | 6.98 | 23.57 | 56.8 | 55.2 |
| Gullies in Crater near Hellas Planitia: ESP_011948_1335 ESP_012014_1335 (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 | -45.9 | 45.9 | -6.0 | -22.2 | 61.0 | 61.2 |
| Light-Toned Gully Feature or Mass Movement: ESP_012417_1435 ESP_012839_1435 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -36.0 | 200. | -5.5 | -20.8 | 51.5 | 46.6 |
| Enigmatic Uplift on the Floor of Echus Chasma: ESP_011715_1800 ESP_012203_1800 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.05 | 279. | 8.06 | -26.2 | 57.0 | 58.9 |
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