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.
| Probing Below the Surface with Impact Craters: ESP_089323_2180 ESP_089600_2180 (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 | 37.68 | 175. | 5.18 | -15.4 | 47.3 | 51.5 |
| Fluvial Valley in Arabia Terra: ESP_090820_2085 ESP_090754_2085 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.33 | 349. | -19. | 3.726 | 63.7 | 61.0 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_090715_1975 ESP_090781_1975 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.07 | 336. | 4.71 | -21.1 | 58.0 | 60.7 |
| Inverted Dendritic Channels in Noachis Terra Crater: ESP_090370_1555 ESP_090581_1555 (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 | -24.1 | 41.6 | 6.89 | -5.62 | 63.2 | 62.6 |
| Alluvial Fan in Coprates Catena Trough: ESP_090308_1650 ESP_090453_1650 (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 | -14.6 | 294. | -16. | 8.504 | 61.8 | 59.4 |
| Layered Mound near Mawrth Vallis: ESP_090359_2045 ESP_090425_2045 (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 | 24.02 | 335. | 8.76 | -7.68 | 55.6 | 57.6 |
| Vent East of Ascraeus Mons: ESP_090375_1925 ESP_090520_1925 (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 | 12.13 | 261. | -5.8 | 10.07 | 56.2 | 55.7 |
| Flow Obstacle in Lobate Debris Apron: ESP_090608_2215 ESP_090107_2215 (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 | 40.89 | 11.8 | 27.4 | 9.221 | 61.0 | 55.7 |
| Terrain around Crater in Terra Sabaea: ESP_090409_2165 ESP_090132_2165 (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 | 36.18 | 50.6 | -6.7 | 5.045 | 59.7 | 55.3 |
| Light-Toned Exposures on Floor of Coprates Chasma: ESP_090413_1645 ESP_090136_1645 (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 | -15.3 | 307. | 4.12 | 18.86 | 60.0 | 60.1 |
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