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.
| 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 |
| 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 |
| An Inverted Channel in Flammarion Crater: ESP_089631_2065 ESP_090330_2065 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.02 | 48.9 | 5.65 | -12.0 | 49.6 | 57.2 |
| Deep in Valles Marineris: ESP_089134_1655 ESP_088633_1655 (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 | -14.3 | 303. | -5.3 | -18.1 | 64.4 | 65.7 |
| Dune Monitoring in Nilosyrtis Mensae: ESP_090092_2110 ESP_089947_2110 (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 | 30.73 | 63.1 | 7.05 | -9.93 | 53.7 | 53.7 |
| Dune Interaction with Residual Polar Ice: ESP_089932_2600 ESP_090156_2600 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.66 | 99.1 | -7.9 | 1.407 | 70.2 | 73.1 |
| Impact Crater Exposing Structure within Lobate Debris Apron: ESP_090278_2205 ESP_089988_2205 (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 | 39.92 | 23.0 | 18.4 | -11.9 | 56.9 | 55.8 |
| Inverted Channel in Noachis Terra: ESP_090252_1600 ESP_090397_1600 (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 | -19.8 | 23.1 | -5.0 | 18.55 | 63.1 | 60.5 |
| Northeast Syrtis Major Planum Ancient Terrain Exposing Diverse Lithologies: ESP_090039_1965 ESP_090606_1965 (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 | 16.39 | 73.1 | -7.1 | 1.975 | 54.1 | 57.3 |
| Mottled Ridged Terrain: ESP_090266_1840 ESP_090688_1840 (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 | 3.703 | 357. | -1.8 | -24.6 | 56.2 | 59.2 |
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