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.
Proposed Landing Site in Nili Fossae: ESP_022878_2010 ESP_022812_2010 (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 | 20.69 | 74.5 | -10. | 11.12 | 50.9 | 50.6 |
Northern Floor of Oudemans Crater: ESP_022871_1705 ESP_023148_1705 (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 | -9.48 | 268. | 4.85 | -23.5 | 33.2 | 33.9 |
Light-Toned Material, Possibly Opal, in Noctis Trough: ESP_023003_1710 ESP_023359_1710 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.07 | 264. | 6.08 | 22.16 | 32.3 | 29.9 |
Well Exposed Layered Deposits and Possible MSL Rover Landing Site: ESP_022707_1505 ESP_022562_1505 (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 | -29.0 | 67.6 | 11.1 | -3.05 | 32.0 | 33.6 |
Fan at Intersection of Valley and Depression Floor: ESP_023036_1310 ESP_023313_1310 (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 | -48.6 | 88.3 | 8.17 | -8.33 | 42.4 | 46.8 |
The Crazy Floor of the Hellas Basin: ESP_023234_1460 ESP_024091_1460 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.5 | 81.5 | 0.57 | 28.11 | 36.3 | 46.4 |
Starburst Spiders at a South Polar Cracked and Gullied Site: ESP_023117_0980 ESP_022998_0980 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.6 | 66.2 | -18. | -2.77 | 70.6 | 67.8 |
Fan-Shaped Deposit in a Valles Marineris Trough: ESP_022949_1650 ESP_030518_1650 (Interval in Earth days: 590) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 299. | -1.6 | 21.10 | 32.0 | 42.9 |
Ultimum Chasma South Polar Layers: ESP_022467_0985 ESP_022586_0985 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.5 | 159. | 2.80 | -12.8 | 61.6 | 63.6 |
Channel Head on Pavonis Mons: ESP_022331_1815 ESP_022753_1815 (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 | 1.616 | 249. | 2.95 | -10.7 | 44.4 | 40.2 |
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