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.
| Hydrated Materials in Nanedi Valles : ESP_053475_1820 ESP_053330_1820 (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 | 1.824 | 310. | 7.39 | -6.72 | 50.5 | 51.4 |
| Terrain along Hebes Mensa: ESP_053265_1785 ESP_053054_1785 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.32 | 283. | 14.8 | 24.92 | 51.6 | 50.5 |
| Northern Continuous Ejecta Boundary of Zunil Crater : ESP_053533_1880 ESP_059995_1880 (Interval in Earth days: 504) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.089 | 166. | 7.85 | -23.4 | 47.3 | 38.7 |
| Dunes Dubbed Kolhar : ESP_053314_2650 ESP_053432_2650 (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 | 84.69 | 0.70 | -8.4 | 6.269 | 60.4 | 60.3 |
| Translucent Ice at Northern Site : ESP_053501_2575 ESP_053554_2575 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.49 | 300. | 7.93 | -7.66 | 55.4 | 56.6 |
| Well-Preserved 5-Kilometer Impact Crater: ESP_053431_1685 ESP_060460_1685 (Interval in Earth days: 548) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.2 | 73.7 | 4.31 | -17.2 | 58.7 | 50.7 |
| Landforms in Utopia Planitia : ESP_053575_2115 ESP_053865_2115 (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 | 31.31 | 96.5 | 5.20 | 26.74 | 40.9 | 40.1 |
| Alluvial Fan in Harris Crater : ESP_053339_1575 ESP_053840_1575 (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 | -22.1 | 66.8 | 5.18 | 23.01 | 66.1 | 64.1 |
| Pitted Cones in Utopia Planitia : ESP_053364_2135 ESP_053219_2135 (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 | 33.11 | 95.0 | 23.6 | 14.25 | 38.2 | 38.7 |
| Candidate Landing Site for 2020 Mission West of Jezero Crater : ESP_053312_1985 ESP_053378_1985 (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 | 18.24 | 77.1 | 24.1 | 3.374 | 41.3 | 43.2 |
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