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.
| Pit in Hephaestus Fossae: ESP_060260_2015 ESP_055209_2015 (Interval in Earth days: 393) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.35 | 127. | 9.79 | 21.07 | 36.4 | 50.9 |
| Pedestal Crater Near Phlegra Montes: ESP_060417_2185 ESP_060351_2185 (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 | 37.95 | 160. | -7.7 | 7.658 | 41.0 | 39.9 |
| Fissure Adjacent to Olympica Fossae: ESP_060282_2055 ESP_060427_2055 (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 | 25.36 | 246. | 1.79 | 18.58 | 37.4 | 36.2 |
| Depressions in Arena Colles: ESP_060301_2040 ESP_060789_2040 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.92 | 88.4 | 0.12 | -18.9 | 37.5 | 40.6 |
| Candidate Landing Site for 2020 Mission Near Jezero Crater: ESP_060341_1985 ESP_060407_1985 (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 | 18.25 | 77.1 | 0.99 | -18.2 | 37.5 | 39.5 |
| Sinuous Gullies and Arcuate Ridges: ESP_060214_1355 ESP_060280_1355 (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 | -44.1 | 311. | 8.88 | -7.81 | 68.5 | 70.4 |
| Sand Dune Changes in Hellespontus Region: ESP_060224_1350 ESP_060290_1350 (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 | -44.8 | 38.7 | 7.87 | -8.66 | 69.3 | 71.1 |
| Chaotic Terrain Near Ravi Vallis: ESP_060451_1790 ESP_061018_1790 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.98 | 316. | 6.53 | 26.02 | 43.5 | 47.1 |
| Gullies: ESP_060298_1340 ESP_060153_1340 (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 | -45.5 | 178. | 7.78 | -7.22 | 70.8 | 69.5 |
| Two Small Cones in Hydraotes Chaos: ESP_060266_1795 ESP_060754_1795 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.34 | 326. | 6.09 | -16.5 | 41.3 | 47.7 |
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