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.
| Depressions with Layering and Faulting : ESP_044141_1730 ESP_044497_1730 (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 | -6.90 | 267. | -23. | -2.42 | 57.2 | 55.9 |
| Mound in Elysium Planitia with Unusual Apron : ESP_043986_1910 ESP_044263_1910 (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 | 10.94 | 174. | 7.11 | -13.5 | 44.9 | 46.8 |
| Low Aspect Ratio Layered Ejecta Crater : ESP_044170_1790 ESP_053809_1790 (Interval in Earth days: 751) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.21 | 193. | 5.51 | -5.00 | 51.8 | 53.1 |
| North Polar Sand Dunes : ESP_044199_2565 ESP_044740_2565 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.58 | 102. | 5.08 | -14.3 | 53.9 | 56.5 |
| Rocky Terrain Near Nili Fossae : ESP_044095_2010 ESP_044662_2010 (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 | 20.82 | 77.5 | 6.46 | 26.09 | 41.3 | 40.2 |
| Candidate Landing Site for 2020 Mission in Nili Fossae : ESP_043963_2020 ESP_043818_2020 (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 | 21.87 | 78.6 | 28.7 | 13.85 | 38.8 | 40.0 |
| Curvilinear Features on the Floor of Huygens Crater : ESP_043885_1665 ESP_043740_1665 (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 | -13.1 | 54.7 | 5.44 | -14.1 | 58.8 | 59.4 |
| Candidate Landing Site for 2020 Mission in Melas Chasma : ESP_044180_1700 ESP_044325_1700 (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 | -9.80 | 283. | -24. | -4.34 | 59.1 | 57.9 |
| Mesa with Ciruclar and Arcuate Scarp Elements : ESP_044114_2315 ESP_044734_2315 (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 | 51.21 | 274. | 1.21 | -28.9 | 41.7 | 45.8 |
| Channel Entering Crater in Sirenum Fossae : ESP_044156_1560 ESP_044512_1560 (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 | -23.6 | 220. | -23. | -2.85 | 68.4 | 67.3 |
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