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.
| Dissected Wrinkle Ridge Surrounded by Viscous Flows in Elysium Planitia: ESP_016572_1875 ESP_016150_1875 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.515 | 157. | 16.0 | 25.58 | 42.9 | 38.9 |
| Light-Toned Layering in Noctis Labyrinthus Pit: ESP_016898_1695 ESP_019377_1695 (Interval in Earth days: 193) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.4 | 261. | -4.2 | -21.4 | 56.2 | 59.9 |
| Cerberus Fossae Region Seen in THEMIS Image: ESP_016651_1895 ESP_044026_1895 (Interval in Earth days: 2134) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.408 | 161. | 2.65 | 18.14 | 43.8 | 44.8 |
| Candidate MSL Landing Site in Northeast Syrtis Major: ESP_016720_1980 ESP_016786_1980 (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 | 17.78 | 76.9 | 2.08 | -17.9 | 41.7 | 43.6 |
| Scalloped Features in Deuteronilus Mensae: ESP_016313_2265 ESP_016590_2265 (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 | 46.17 | 23.3 | 8.14 | -8.96 | 44.5 | 44.6 |
| Fresh 6-Kilometer Diameter Crater South of Coprates Chasma: ESP_016422_1625 ESP_017345_1625 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.1 | 296. | -0.6 | 9.867 | 55.4 | 62.6 |
| Light-Toned Layering in Coprates Catena Trough: ESP_016857_1645 ESP_017569_1645 (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 | -15.1 | 301. | 0 | 9.274 | 58.6 | 62.2 |
| Wrinkle Ridges in Hesperia Planum: ESP_016455_1535 ESP_016811_1535 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.2 | 117. | -5.9 | 7.118 | 62.1 | 65.3 |
| Well-Preserved 30-Kilometer Diameter Impact Crater with Bedrock Exposures: ESP_016760_1585 ESP_017538_1585 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 70.1 | -2.0 | -13.5 | 62.0 | 67.8 |
| Potential Rhythmic Layering in East Gale Crater with Hydrated Signature: ESP_016375_1750 ESP_016520_1750 (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 | -5.15 | 138. | 1.01 | 18.09 | 48.0 | 48.2 |
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