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.
| 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 |
| Very Well-Preserved 40-Kilometer Crater in Noachis Terra: ESP_026229_1540 ESP_026374_1540 (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 | -25.7 | 34.5 | -4.8 | 10.81 | 68.8 | 68.6 |
| 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 |
| Sand Dunes in Crater: ESP_026230_2450 ESP_025729_2450 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 64.80 | 351. | 7.20 | -2.81 | 47.6 | 50.3 |
| Heavily Dissected Ancient Bedrock: ESP_026319_1740 ESP_062846_1740 (Interval in Earth days: 2846) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.17 | 94.7 | -3.5 | -16.0 | 55.9 | 58.6 |
| Well-Preserved Mid-Latitude Impact Crater: ESP_026572_2220 ESP_027060_2220 (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 | 41.44 | 21.4 | -2.2 | -20.8 | 41.1 | 44.4 |
| Well-Preserved Impact Crater: ESP_026238_1520 ESP_053692_1525 (Interval in Earth days: 2140) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.9 | 149. | -6.6 | 13.05 | 70.5 | 69.2 |
| Secondary Ray Chains Closest to Gratteri Crater: ESP_026302_1615 ESP_026447_1615 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.3 | 199. | 4.41 | 20.29 | 63.4 | 62.9 |
| Sharp-Rimmed Crater on Northern Plains: ESP_026383_2465 ESP_026673_2465 (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 | 66.00 | 137. | -7.2 | 4.831 | 49.1 | 48.3 |
| Abrupt Terrain Changes Near Adamas Labyrinthus: ESP_026437_2180 ESP_087295_2180 (Interval in Earth days: 4742) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.85 | 106. | 3.21 | -6.09 | 40.2 | 43.0 |
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