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.
| 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 |
| Northern Section of Dunes Dubbed South Beach : ESP_053369_2550 ESP_053105_2550 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.98 | 311. | -3.9 | 16.93 | 54.1 | 52.1 |
| Aeolian Processes West of Gordii Dorsum: ESP_053228_1825 ESP_053373_1825 (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 | 2.636 | 214. | 0.81 | 14.34 | 50.3 | 49.5 |
| 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 |
| 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 |
| 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 |
| Dark Materials on Olympus Mons: ESP_012548_1980 ESP_013049_1980 (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 | 17.55 | 216. | -2.9 | 20.20 | 63.7 | 59.8 |
| Small Field of Eroding Dunes : ESP_053034_1645 ESP_053179_1645 (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 | -15.4 | 114. | -7.3 | 5.87 | 61.8 | 61.2 |
| Candidate ExoMars Landing Site in Oxia Palus: ESP_053184_1980 ESP_061980_1980 (Interval in Earth days: 685) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.82 | 336. | -26. | -8.44 | 45.5 | 45.3 |
| Gale Crater Mesa: ESP_052954_1740 ESP_053020_1740 (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 | -5.74 | 137. | -6.3 | -28.5 | 55.1 | 56.9 |
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