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.
| Northwest Wall of Juventae Chasma: ESP_013244_1760 ESP_030228_1760 (Interval in Earth days: 1323) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.14 | 296. | 0 | 10.99 | 46.6 | 50.0 |
| Well-Preserved Impact Crater: ESP_013238_1945 ESP_013871_1945 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.53 | 98.5 | -0.1 | -22.9 | 57.4 | 51.3 |
| Unusual Dune Form along Inner Small Crater Rim: ESP_013909_1145 ESP_014041_1145 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -65.1 | 151. | -0.4 | -20.7 | 51.9 | 54.5 |
| Crater Wall Carving in MOC Image E0300089: ESP_013828_1360 ESP_013683_1360 (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 | -43.4 | 196. | 18.3 | 8.46 | 37.6 | 38.3 |
| South Polar Layered Deposits Exposed in Promethei Lingula: ESP_013832_0975 ESP_013647_0975 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.5 | 112. | -3.5 | 14.29 | 64.8 | 62.0 |
| Kaiser Crater Dunes with Channels: ESP_013083_1325 ESP_013017_1325 (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 | -47.2 | 19.4 | -8.1 | 8.076 | 44.5 | 44.0 |
| Small Rayed Crater in Syrtis Major Planum: ESP_012791_1910 ESP_012857_1910 (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 | 10.67 | 62.2 | 4.22 | -17.8 | 58.5 | 59.5 |
| Wrinkle Ridge in Lunae Palus: ESP_014022_1950 ESP_014167_1950 (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 | 14.94 | 294. | -7.9 | 7.828 | 48.7 | 45.9 |
| Light-Toned Material in a Crater in Terra Cimmeria: ESP_013750_1440 ESP_021543_1440 (Interval in Earth days: 608) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -35.8 | 166. | -2.2 | 19.05 | 36.5 | 43.0 |
| Layered Material Exposed on Crater Floor: ESP_013017_2150 ESP_013518_2150 (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 | 34.69 | 8.85 | 6.51 | 22.48 | 72.6 | 67.8 |
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