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.
| Impact Crater on East Side of Gale Crater: ESP_026502_1750 ESP_026647_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 | -5.06 | 138. | -3.6 | 13.91 | 55.8 | 55.0 |
| Bedrock Stratigraphy Exposed in Crater Wall: ESP_026333_2015 ESP_026478_2015 (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 | 21.35 | 68.7 | 0.94 | 15.99 | 42.4 | 41.5 |
| Exposed Bedrock in Crater Central Uplift off Thaumasia Planum: ESP_026496_1610 ESP_027485_1610 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.0 | 304. | -6.5 | 5.269 | 65.1 | 64.1 |
| Light-Toned Layering along Floor of Small Trough Near Juventae Chasma: ESP_026272_1730 ESP_026628_1730 (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 | -6.84 | 298. | -5.3 | 6.566 | 56.2 | 56.6 |
| Cones and Crater in Isidis Planitia: ESP_026372_1920 ESP_026438_1920 (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 | 11.64 | 83.7 | 18.6 | -2.63 | 44.7 | 46.6 |
| Features of Large Lobe Northwest of Pavonis Mons: ESP_026564_1850 ESP_027553_1850 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.068 | 244. | -7.0 | 7.531 | 50.4 | 50.7 |
| Dune Motion in Northern Plains Rampart Crater: ESP_026259_2350 ESP_026549_2350 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.64 | 284. | -5.6 | 11.61 | 44.1 | 42.7 |
| Contacts between Yardang-Forming Material and Platy Flow Material: ESP_026541_1840 ESP_026607_1840 (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 | 3.813 | 152. | 5.15 | -16.8 | 50.2 | 51.9 |
| Pit in Syria Planum: ESP_026247_1650 ESP_051987_1650 (Interval in Earth days: 2006) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.6 | 260. | 8.36 | -6.82 | 60.4 | 55.1 |
| Samara Valles and Mars 6 Descent Area: ESP_026376_1555 ESP_036991_1555 (Interval in Earth days: 827) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.0 | 340. | -2.2 | -20.7 | 68.0 | 67.4 |
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