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.
Crater with Central Pit in Tyrrhena Terra: ESP_019620_1680 ESP_036050_1680 (Interval in Earth days: 1280) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 106. | -8.3 | 16.38 | 58.7 | 60.8 |
Contact between Wallrock and Light-Toned Layering in West Candor Chasma: ESP_019719_1750 ESP_020075_1750 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.90 | 282. | -8.7 | 6.86 | 56.3 | 54.8 |
The Beautiful Arc of a Dune: ESP_019992_1340 ESP_020269_1340 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -45.5 | 33.9 | 8.50 | -14.2 | 69.5 | 67.2 |
Eastern Edge of Eberswalde Crater Delta in Possible MSL Rover Landing Site: ESP_019757_1560 ESP_020034_1560 (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 | -23.8 | 326. | 7.74 | -16.3 | 61.7 | 61.4 |
Striated Walls in Arnus Vallis: ESP_019964_1935 ESP_024421_1935 (Interval in Earth days: 347) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.19 | 70.2 | 13.7 | -4.81 | 53.1 | 36.3 |
Possible MSL Rover Landing Site in Holden Crater: ESP_019823_1530 ESP_019889_1530 (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 | -26.5 | 325. | 8.09 | -12.7 | 62.3 | 63.3 |
Lower Northwest Portion of Mound in Gale Crater: ESP_019698_1750 ESP_019988_1750 (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 | -4.88 | 137. | -22. | 13.72 | 57.5 | 54.3 |
Central Peak of Crater in Tyrrhena Terra: ESP_019951_1510 ESP_028509_1510 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.6 | 72.1 | -5.4 | 11.57 | 63.1 | 63.5 |
Lava Channel in Tharsis Region: ESP_019694_2005 ESP_019839_2005 (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 | 20.27 | 242. | -5.5 | 11.06 | 53.2 | 53.0 |
Sinuous Ridges : ESP_019677_1585 ESP_019743_1585 (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 | -21.1 | 350. | 5.41 | -16.1 | 61.2 | 62.3 |
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