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.
| Gullies in Dunes: ESP_014151_1325 ESP_021509_1325 (Interval in Earth days: 573) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.1 | 19.5 | 5.65 | -10.1 | 42.1 | 48.1 |
| Possible Monohydrated Sulfate-Rich Terrain in Columbus Crater: ESP_014039_1510 ESP_021832_1510 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.7 | 194. | 7.74 | 26.60 | 33.9 | 38.3 |
| Enigmatic Pit in Southern Cerberus Palus: ESP_012893_1775 ESP_013605_1775 (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 | -2.47 | 160. | -6.3 | 12.12 | 51.7 | 42.2 |
| Possible Olivine-Rich Terrain in Ejecta of a Gullied Crater: ESP_012761_1430 ESP_013117_1430 (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 | -36.8 | 167. | 6.94 | 17.27 | 45.6 | 40.1 |
| Bedrock Exposures in Central Uplift of Large Crater North of Eos Chasma: ESP_013151_1685 ESP_013573_1685 (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 | -11.2 | 317. | -0.6 | -17.0 | 44.8 | 40.9 |
| Strike Slip Fault in Amazonis Planitia: ESP_012799_1990 ESP_013076_1990 (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 | 18.75 | 203. | 1.92 | -21.6 | 63.2 | 63.0 |
| Diverse Layers and Morphologies in North Rim of Hellas Planitia: ESP_013490_1525 ESP_058166_1530 (Interval in Earth days: 3481) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.3 | 64.2 | -5.3 | 5.215 | 37.6 | 30.5 |
| Floor of Mawrth Vallis: ESP_014007_2030 ESP_022578_2030 (Interval in Earth days: 668) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.98 | 341. | 9.10 | 25.33 | 53.5 | 54.6 |
| Warrego Valles Headwater Region: ESP_013153_1390 ESP_013298_1390 (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 | -40.6 | 266. | -5.4 | 6.316 | 42.0 | 39.7 |
| Crater between Branches of Athabasca Valles: ESP_013460_1900 ESP_013737_1900 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.648 | 157. | 4.42 | -23.9 | 51.5 | 50.0 |
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