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 Scarps and Terraces: ESP_087921_2055 ESP_087855_2055 (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 | 25.07 | 301. | -29. | -8.33 | 46.5 | 44.4 |
| Utopia Planitia Terrain: ESP_087875_2200 ESP_088310_2200 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.68 | 113. | -5.7 | 11.81 | 43.1 | 42.1 |
| Athabasca Valles: ESP_087834_1895 ESP_088401_1895 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.534 | 156. | -2.1 | -25.3 | 49.0 | 52.7 |
| Terrain Northeast of Pollack Crater: ESP_087786_1735 ESP_088498_1735 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.28 | 27.9 | 3.19 | -8.79 | 56.9 | 59.9 |
| Layering in Heavily Cratered Lucus Planum Terrain: ESP_087820_1755 ESP_088110_1755 (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 | -4.46 | 179. | 0.91 | 19.03 | 56.1 | 56.1 |
| Terrain Northeast of Airy Crater: ESP_087800_1780 ESP_088868_1780 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.10 | 5.00 | 6.21 | -8.90 | 54.3 | 57.9 |
| Isolated Dune Field in Crater Northwest of Syrtis Major Planum: ESP_087903_2050 ESP_089050_2050 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.85 | 71.6 | -17. | 0.922 | 45.3 | 47.0 |
| Light-Toned Fractured Material West of Nectaris Montes: ESP_087710_1655 ESP_087644_1655 (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 | -14.4 | 303. | 1.75 | 21.48 | 61.6 | 59.9 |
| Crater near Marte Vallis: ESP_087701_1980 ESP_088268_1980 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.73 | 184. | 6.84 | -6.87 | 44.6 | 47.5 |
| Topographic and Albedo Feature in Western Arcadia Planitia: ESP_087873_2190 ESP_088308_2190 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.78 | 167. | -3.9 | 13.58 | 42.9 | 41.9 |
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