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.
| Kasei Valles Alluvial Fans and Flood Terrace: ESP_089820_2025 ESP_089675_2025 (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 | 22.03 | 290. | -0.2 | -16.9 | 51.7 | 52.1 |
| Crater in Arabia Terra: ESP_089804_2205 ESP_090160_2205 (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 | 39.96 | 7.23 | -21. | -7.62 | 54.5 | 57.6 |
| Debris Apron in Phlegra Montes: ESP_089864_2285 ESP_090009_2285 (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 | 47.97 | 165. | -0.6 | 11.32 | 55.2 | 56.1 |
| Exposed Layers in Olympia Mensae Icy Outliers: ESP_089774_2545 ESP_089787_2545 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.13 | 95.1 | -4.3 | 10.35 | 64.8 | 63.9 |
| Features around Crater in Terra Sabaea: ESP_089842_2165 ESP_089565_2165 (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 | 36.09 | 50.5 | -24. | -6.66 | 54.5 | 50.2 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_089726_1975 ESP_089225_1975 (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 | 17.14 | 336. | 11.0 | -14.0 | 50.8 | 50.8 |
| Iani Chaos: ESP_089660_1780 ESP_089238_1780 (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 | -1.75 | 341. | -6.6 | 6.11 | 57.5 | 56.6 |
| Sample of Scalloped Terrain West of Erebus Montes: ESP_089349_2195 ESP_089072_2195 (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 | 39.37 | 187. | -8.3 | 14.20 | 48.9 | 44.9 |
| Light-Toned Mesas in Arcadia Planitia: ESP_089560_2260 ESP_089336_2260 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.44 | 183. | 12.9 | -21.3 | 49.9 | 50.8 |
| Possible Vent in Young Lava Flows in Elysium Region: ESP_089244_2090 ESP_089534_2090 (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 | 28.68 | 174. | 4.31 | 28.13 | 47.1 | 46.6 |
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