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.
| Layered Deposits: ESP_073865_1725 ESP_066149_1725 (Interval in Earth days: 601) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.39 | 282. | 4.29 | 28.47 | 55.1 | 45.3 |
| Dune Monitoring in Candidate ExoMars Landing Site in Mawrth Vallis: ESP_073533_2010 ESP_073467_2010 (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 | 20.85 | 342. | -2.1 | 16.69 | 63.1 | 61.1 |
| Curved Ridges in Aeolis Planum: ESP_073738_1810 ESP_065745_1810 (Interval in Earth days: 623) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.857 | 148. | -4.1 | 6.072 | 57.9 | 54.4 |
| Landslides inside Impact Crater: ESP_073749_1860 ESP_073815_1860 (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 | 5.745 | 207. | 7.31 | -11.9 | 58.3 | 59.8 |
| Eroding Deposits on Floor of Barnard Crater: ESP_073636_1185 ESP_073979_1185 (Interval in Earth days: 26) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -61.0 | 62.0 | 4.12 | -13.5 | 66.5 | 61.8 |
| Aeolis Dorsa Deltaic Lobes: ESP_073817_1735 ESP_074819_1735 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.44 | 153. | -7.6 | 27.7 | 56.4 | 45.6 |
| Ares Vallis Landform: ESP_073639_1950 ESP_073916_1950 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 14.59 | 329. | -4.6 | -18.6 | 61.8 | 63.7 |
| Cliffs of Crumbling, Layered Sediments: ESP_072533_1680 ESP_078309_1680 (Interval in Earth days: 450) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.9 | 288. | -0.4 | -20.4 | 60.3 | 57.4 |
| Shallow Vent East of Olympus Mons: ESP_073181_1970 ESP_073115_1970 (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 | 16.78 | 232. | -0.3 | 20.53 | 59.3 | 57.0 |
| Region Dubbed Troy: ESP_073472_0950 ESP_073471_0950 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.0 | 259. | -8.9 | 18.63 | 82.6 | 80.4 |
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