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.
Many Small Cones in Amazonis Planitia: ESP_021990_1985 ESP_022412_1990 (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 | 18.78 | 198. | -4.5 | -18.4 | 59.5 | 56.0 |
Well-Preserved 5-Kilometer Diameter Impact Crater: ESP_021767_1315 ESP_022400_1315 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.2 | 173. | 6.74 | -8.25 | 43.6 | 40.1 |
Well-Preserved Flow-Ejecta Crater East of Juventae Chasma: ESP_021683_1735 ESP_057933_1740 (Interval in Earth days: 2824) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.25 | 301. | 5.27 | 14.08 | 47.4 | 34.0 |
Hematite in Eos Chasma: ESP_021775_1665 ESP_022408_1665 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 311. | -3.6 | -23.2 | 44.4 | 38.4 |
Central Uplift with Layers and Clays: ESP_021688_1325 ESP_021754_1325 (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 | -47.2 | 170. | 2.61 | -14.9 | 44.6 | 45.1 |
Mounds North of Simud Valles Region Chaos: ESP_021880_1950 ESP_030359_1950 (Interval in Earth days: 661) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.75 | 320. | 4.40 | -21.0 | 57.2 | 60.9 |
Northern Part of Asimov Crater Ring Trough: ESP_021694_1330 ESP_021760_1330 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.4 | 4.90 | 21.1 | 4.178 | 42.9 | 43.4 |
Mesas and Buttes of Hydraotes Chaos: ESP_021893_1805 ESP_031163_1805 (Interval in Earth days: 722) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.634 | 327. | 3.40 | 22.57 | 48.7 | 42.4 |
Bedform Changes in Aureum Chaos: ESP_021906_1765 ESP_022183_1765 (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 | -3.64 | 333. | -1.9 | -28.1 | 46.7 | 45.5 |
Fractures and Uplifted Portion of Floor of Echus Chasma: ESP_021908_1810 ESP_021842_1810 (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 | 0.856 | 279. | -17. | 4.9 | 50.1 | 49.2 |
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