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.
| Flow Associated with Hrad Vallis: ESP_035798_2140 ESP_037077_2140 (Interval in Earth days: 100) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.85 | 140. | 5.93 | 24.47 | 42.8 | 50.6 |
| Cerberus Region Intra-Crater Dune Field: ESP_035929_1885 ESP_036285_1885 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.525 | 169. | -8.9 | 11.89 | 51.4 | 50.5 |
| Exposure of North Polar Layered Deposits: ESP_035605_2660 ESP_036013_2660 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.87 | 328. | -0.4 | 9.648 | 60.9 | 62.4 |
| Candidate Landing Site for InSight: ESP_035785_1840 ESP_036062_1840 (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 | 4.050 | 138. | 21.9 | 0.533 | 51.0 | 53.0 |
| Candidate Landing Site for 2020 Mission in West Meridiani Planum: ESP_035975_1795 ESP_036252_1795 (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 | -0.58 | 351. | 23.9 | 4.956 | 53.6 | 55.1 |
| High-Latitude Dune Footprints: ESP_035684_2650 ESP_035922_2650 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.93 | 339. | 0.50 | -13.5 | 60.3 | 62.0 |
| North Polar Layered Deposits Exposure: ESP_035652_2660 ESP_035943_2660 (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 | 85.90 | 122. | 1.50 | -13.9 | 61.0 | 62.7 |
| Dark-Capped Plain and Hills in Western Arabia Region Intercrater Terrain: ESP_035883_1995 ESP_036806_1995 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.50 | 342. | -1.6 | 17.24 | 46.6 | 48.9 |
| Crater Ejecta in Terra Sirenum: ESP_035875_1470 ESP_035941_1470 (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 | -32.8 | 206. | 10.8 | -8.45 | 75.4 | 76.3 |
| Monitor Dunes in Crater Northeast of Syrtis Major: ESP_035919_2005 ESP_035774_2005 (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 | 20.25 | 79.1 | 8.77 | -9.01 | 45.6 | 46.6 |
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