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.
Cataracts at the Proximal Ends of Distributaries in Athabasca Valles: ESP_011891_1885 ESP_012313_1885 (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 | 8.235 | 154. | -7.7 | -19.1 | 60.0 | 60.9 |
Shalbatana Vallis Layering: ESP_011740_1830 ESP_019454_1830 (Interval in Earth days: 601) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.120 | 316. | 8.28 | -8.81 | 57.4 | 54.2 |
Gully Fans with Age Constraint: ESP_012314_1450 ESP_012459_1450 (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 | -34.8 | 131. | 3.91 | 17.39 | 52.2 | 49.0 |
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 |
Alcove in East Candor Chasma Layered Deposits: ESP_011965_1725 ESP_012242_1725 (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 | -7.47 | 293. | 27.3 | 0.012 | 54.0 | 54.8 |
Dunes in the Western Nereidum Montes: ESP_012202_1390 ESP_013046_1390 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -40.4 | 309. | -0.6 | -22.5 | 55.1 | 44.6 |
Cones and Mounds in Olympus Mons Aureole: ESP_012363_2145 ESP_012996_2145 (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 | 34.19 | 224. | 4.44 | -14.0 | 72.2 | 73.5 |
Layered Deposit in an Arabia Region Crater: ESP_012385_1825 ESP_030648_1825 (Interval in Earth days: 1423) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.668 | 350. | -23. | -0.71 | 58.9 | 50.7 |
Oudemans Crater Central Uplift: ESP_011676_1700 ESP_028449_1700 (Interval in Earth days: 1307) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.84 | 267. | -22. | 7.568 | 59.1 | 56.2 |
Gullies Associated with Resistant Layers: ESP_012486_1220 ESP_013185_1220 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -57.6 | 118. | 7.81 | -17.9 | 55.0 | 48.2 |
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