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.
| Ridges and Fractures in Sublimation-Pit Crater with Hale Crater Ejecta: ESP_082620_1415 ESP_082844_1415 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.0 | 319. | -7.3 | 22.81 | 57.5 | 51.8 |
| Possible Scour Pits adjacent to Yardangs in Southwest Olympus Mons: ESP_082597_1890 ESP_082821_1890 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.852 | 221. | -7.1 | 26.60 | 61.0 | 58.3 |
| Possible Spatter Cones East of Arsia Mons: ESP_082873_1715 ESP_083440_1715 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.45 | 246. | -0.0 | 0.453 | 54.6 | 49.4 |
| Uphill Facing Scarps and Lobate Deformation on Slope: ESP_082523_2085 ESP_082602_2085 (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 | 28.12 | 78.9 | 6.50 | 29.15 | 67.2 | 65.9 |
| Exposed Crater Floor Materials in Western Arabia Terra: ESP_082552_1835 ESP_090648_1835 (Interval in Earth days: 631) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.618 | 10.1 | 7.89 | -24.4 | 58.3 | 59.1 |
| Layered Deposits on Playfair Crater: ESP_082716_1020 ESP_083362_1020 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -78.0 | 234. | -8.2 | -2.63 | 70.9 | 61.4 |
| Pedestal Crater near Crommelin Crater: ESP_082566_1830 ESP_083212_1830 (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 | 3.162 | 348. | -4.3 | 3.227 | 59.2 | 56.2 |
| Ridges Associated with Dipping Layers in Reull Vallis: ESP_082839_1390 ESP_083129_1390 (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 | -40.5 | 99.1 | -0.7 | 17.03 | 54.2 | 48.5 |
| Features Southeast of Ostrov Crater: ESP_082804_1520 ESP_083015_1520 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 332. | 5.33 | -10.5 | 52.8 | 51.3 |
| Resistant Layer in Medusae Fossae Formation: ESP_082729_1830 ESP_083230_1830 (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 | 2.727 | 217. | -6.6 | 0.505 | 58.9 | 56.0 |
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