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.
| Lava and Streamlined Forms in Athabasca Valles: ESP_042167_1890 ESP_052294_1890 (Interval in Earth days: 789) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.141 | 156. | 7.63 | -5.94 | 37.4 | 44.1 |
| Daedalia Planum Lava Flows: ESP_042296_1545 ESP_042362_1545 (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 | -25.1 | 236. | 23.7 | 0.587 | 51.3 | 53.7 |
| Dense Gullies in East Argyre Region: ESP_042372_1325 ESP_051378_1325 (Interval in Earth days: 701) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.0 | 327. | -5.8 | 25.72 | 69.4 | 69.3 |
| Aram Chaos Slope Monitoring Site: ESP_042490_1835 ESP_042635_1835 (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 | 3.297 | 339. | -7.2 | 5.79 | 41.7 | 41.7 |
| Mounds on Crater Floor Southwest of Shatskiy Crater: ESP_042279_1465 ESP_042925_1465 (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 | -33.2 | 344. | -2.0 | 22.24 | 57.9 | 64.9 |
| Contacts between Isidis Planitia Olivine-Rich Units and Other Units: ESP_042341_1835 ESP_042631_1835 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.261 | 86.6 | -0.3 | 23.42 | 40.1 | 40.2 |
| 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 |
| East Endeavour Crater Dune Field: ESP_042674_1775 ESP_042740_1775 (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 | -2.32 | 354. | 7.30 | -16.8 | 44.2 | 46.5 |
| Candidate Landing Site for 2020 Mission in Eridania Region: ESP_042219_1515 ESP_042285_1515 (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 | -28.2 | 181. | 4.52 | -18.5 | 53.4 | 55.8 |
| Floor of Uzboi Vallis South of Nirgal Vallis: ESP_042082_1495 ESP_042016_1495 (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 | -30.0 | 322. | -4.5 | 16.71 | 53.1 | 50.7 |
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