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.
| Well-Preserved Crater in Margaritifer Terra: ESP_016407_1675 ESP_016763_1675 (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 | -12.5 | 345. | -0.5 | 12.61 | 52.5 | 55.3 |
| 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 |
| Fretted Valley Outlet: ESP_016391_2195 ESP_016668_2195 (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 | 38.96 | 56.1 | -0.8 | -19.4 | 42.2 | 43.3 |
| 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 |
| Gullied Crater Wall: ESP_016343_2350 ESP_017978_2350 (Interval in Earth days: 128) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.87 | 284. | -3.8 | 7.591 | 49.3 | 44.4 |
| Well-Preserved Impact Crater with Central Peak in Acidalia Planitia: ESP_016777_2175 ESP_016289_2175 (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 | 37.17 | 320. | -17. | 5.433 | 42.8 | 41.5 |
| Melas Fossae: ESP_016541_1520 ESP_019877_1520 (Interval in Earth days: 260) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 288. | 6.46 | 28.65 | 63.3 | 60.7 |
| Cratered Mounds in Galaxias Colles: ESP_016691_2175 ESP_018260_2175 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.23 | 146. | 0 | 27.19 | 41.3 | 40.5 |
| Ridges and Fill Material Among Knobs on West Flank of Arsia Mons: ESP_016833_1715 ESP_019035_1715 (Interval in Earth days: 171) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.53 | 235. | -1.7 | 13.23 | 54.3 | 57.3 |
| 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 |
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