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.
| Features: ESP_090258_1905 ESP_090680_1905 (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 | 10.20 | 215. | -2.5 | -23.7 | 55.4 | 59.4 |
| 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 |
| Depression on Crater Floor in Terra Cimmeria: ESP_090261_1605 ESP_090406_1605 (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 | -19.3 | 137. | -7.6 | 16.44 | 63.0 | 60.4 |
| 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 |
| 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 |
| Light-Toned Exposures in Capri Chasma: ESP_090215_1670 ESP_090149_1670 (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 | -12.9 | 312. | -3.4 | 16.26 | 60.6 | 59.3 |
| Mesas in Arcadia Planitia: ESP_090180_2265 ESP_090325_2265 (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 | 46.27 | 179. | 0.44 | 14.76 | 58.9 | 59.9 |
| Baetis Chasma Transect: ESP_090176_1755 ESP_090598_1755 (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 | -4.49 | 294. | 5.96 | -5.77 | 57.3 | 58.0 |
| 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 |
| Possible Skylight Showing Thermal Anomaly in Young Lava Flows: ESP_089930_1890 ESP_090286_1890 (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 | 8.718 | 169. | -5.8 | 16.74 | 54.6 | 54.1 |
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