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.
| Ismenius Cavus Channel: ESP_089342_2145 ESP_090252_2145 (Interval in Earth days: 71) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.01 | 17.7 | 5.30 | -17.5 | 47.4 | 58.3 |
| Planned ExoMars Landing Ellipse Imaging in Oxia Planum: ESP_089581_1995 ESP_089291_1995 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.24 | 335. | 3.28 | -24.9 | 50.3 | 51.5 |
| Dune Interaction with Residual Polar Ice: ESP_089286_2595 ESP_089405_2595 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.46 | 89.3 | 3.05 | -13.8 | 61.3 | 63.6 |
| Exposure of North Polar Layered Deposits: ESP_089303_2605 ESP_089962_2605 (Interval in Earth days: 52) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.27 | 345. | 0.31 | 14.90 | 62.1 | 69.6 |
| Avalanche Scarp: ESP_089280_2640 ESP_089386_2640 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.76 | 236. | 6.42 | -8.01 | 63.6 | 65.4 |
| Mamers Valles: ESP_089329_2175 ESP_089606_2175 (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 | 37.21 | 13.9 | -10. | -29.1 | 48.8 | 52.9 |
| Dune Interaction with Residual Polar Ice: ESP_089589_2600 ESP_089470_2600 (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 | 79.63 | 97.9 | 1.02 | 16.15 | 64.9 | 62.5 |
| Characterize Possilbe Rotorcraft Landing Site: ESP_089283_2205 ESP_089362_2205 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.97 | 189. | -7.1 | 19.14 | 48.3 | 46.5 |
| Skylight Candidate near Elysium Mons: ESP_089522_2090 ESP_089667_2090 (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 | 28.91 | 145. | -3.6 | 11.04 | 49.5 | 49.3 |
| Fan-Shaped Deposit in Arcadia Planitia: ESP_089428_2200 ESP_089494_2200 (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 | 39.86 | 188. | 6.33 | -9.62 | 48.3 | 50.2 |
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