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 Layered Deposits Exposed along Ladon Valles Floor: ESP_033642_1585 ESP_033787_1585 (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 | -21.0 | 330. | -3.9 | 12.32 | 52.4 | 53.4 |
| Possible Smectite Deposits in Northwest Hellas Region: ESP_033652_1580 ESP_041907_1580 (Interval in Earth days: 643) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.6 | 57.2 | 2.99 | 20.83 | 52.5 | 43.8 |
| Pit South of Arsia Mons: ESP_033342_1660 ESP_050089_1660 (Interval in Earth days: 1305) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.8 | 240. | -0.3 | -8.91 | 43.9 | 32.6 |
| High-Lava Mark in Kasei Valles: ESP_033617_1990 ESP_034316_1990 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.64 | 285. | 20.6 | -9.79 | 36.5 | 42.1 |
| 12-Kilometer Diameter Crater with Multiple Pronounced Internal Morphologies: ESP_033317_1945 ESP_033462_1945 (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 | 14.33 | 199. | -1.3 | 12.06 | 37.2 | 36.6 |
| Flow Boundary in Phlegra Dorsa: ESP_033608_2085 ESP_034109_2085 (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 | 28.33 | 172. | -2.7 | 21.29 | 39.9 | 37.9 |
| Low Shield Volcano Fissure Vent in Syria Planum: ESP_033605_1645 ESP_033750_1645 (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 | -15.2 | 259. | 7.01 | 22.99 | 47.7 | 48.6 |
| Flow on Floor of Isil Crater: ESP_033585_1525 ESP_033730_1525 (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 | -27.3 | 87.8 | -5.6 | 9.704 | 55.7 | 56.9 |
| Differential Compaction around a Crater Peak: ESP_033108_1800 ESP_033253_1800 (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 | -0.12 | 146. | 6.22 | 18.28 | 36.0 | 36.3 |
| Western Portion of Possible Multiple Impact in Arabia Terra: ESP_033272_1840 ESP_033417_1840 (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 | 4.045 | 349. | -3.5 | 10.60 | 37.5 | 37.5 |
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