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.
| Light-Toned Exposures in Capri Chasma: ESP_090004_1670 ESP_089938_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 | -13.0 | 312. | -5.2 | 15.64 | 61.4 | 60.1 |
| Fracture near Double Crater: ESP_090204_1700 ESP_090349_1700 (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 | -9.67 | 251. | 6.04 | 28.44 | 58.8 | 56.7 |
| 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 |
| 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 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 |
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_090006_2240 ESP_090362_2240 (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 | 43.48 | 249. | 2.39 | 19.01 | 55.5 | 59.1 |
| 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 |
| Ismenius Cavus Channel: ESP_089975_2145 ESP_090542_2145 (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 | 34.06 | 17.8 | -4.5 | 9.44 | 53.9 | 59.6 |
| 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 |
| 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 |
Page 6 of 881 (8,805 images) | |||||