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.
| Terrain Contacts in Argyre Region: ESP_042359_1295 ESP_050996_1295 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -50.1 | 322. | -3.6 | -19.7 | 71.4 | 68.2 |
| Western Edge of Marth Crater : ESP_042252_1930 ESP_042753_1930 (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 | 12.63 | 355. | -1.8 | 11.25 | 38.5 | 39.4 |
| From Ares 3 to Ares 4: ESP_042014_1760 ESP_042647_1760 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.96 | 15.1 | 3.24 | -28.0 | 38.9 | 47.4 |
| Nested Channels near Hellas: ESP_042433_1535 ESP_042855_1535 (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 | -26.3 | 98.5 | -1.4 | -21.2 | 55.5 | 61.9 |
| Western Medusa Fossae Formation: Dust and Dunes: ESP_041864_1745 ESP_050725_1745 (Interval in Earth days: 691) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.43 | 150. | 2.13 | 25.91 | 37.9 | 33.3 |
| Candidate Landing Site for 2020 Mission in Oxia Palus Region: ESP_041989_1980 ESP_055175_1980 (Interval in Earth days: 1027) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.81 | 335. | -6.6 | 20.39 | 38.9 | 50.2 |
| Morphometry of Secondary Impact Craters: ESP_041890_1800 ESP_042035_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 | -0.18 | 160. | 3.15 | 17.36 | 37.0 | 37.0 |
| Slope Streak Cluster Formation: ESP_041968_2075 ESP_042614_2075 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.37 | 187. | -1.5 | 22.30 | 41.5 | 37.6 |
| Daedalia Planum Lava Flows: ESP_041861_1575 ESP_049509_1575 (Interval in Earth days: 596) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -22.3 | 234. | 7.61 | -4.70 | 44.4 | 30.8 |
| Contact between Isidis Planitia Olivine-Rich Unit and Ejecta of Crater: ESP_041919_1835 ESP_042064_1835 (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 | 3.439 | 86.8 | 16.4 | 28.67 | 35.7 | 35.5 |
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