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.
| A Mysterious Fractured Depression on Mars: ESP_071541_2200 ESP_071607_2200 (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 | 39.45 | 6.64 | 8.43 | -8.12 | 47.0 | 48.7 |
| Possible Mud Volcanoes on Mars: ESP_071462_2245 ESP_071528_2245 (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 | 44.27 | 2.72 | 8.11 | -7.03 | 47.1 | 48.7 |
| Collapse Terrain South of Orson Welles Crater: ESP_071675_1780 ESP_070818_1780 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.23 | 314. | 4.03 | -16.6 | 57.4 | 61.0 |
| Athabasca Valles: ESP_071628_1890 ESP_071483_1890 (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 | 9.072 | 155. | 8.15 | -6.45 | 52.3 | 53.6 |
| Potential Channel in Gusev Crater: ESP_071812_1660 ESP_071891_1660 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.6 | 175. | -3.7 | 28.34 | 63.4 | 60.8 |
| North Polar Layered Deposits: ESP_071809_2685 ESP_071531_2685 (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 | 88.70 | 260. | -28. | -20.7 | 70.4 | 67.3 |
| Crater in Hydraotes Chaos: ESP_071635_1810 ESP_072070_1810 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.777 | 326. | 0.01 | 28.11 | 56.4 | 53.8 |
| ExoMars Landing Site within Oxia Planum: ESP_071951_1980 ESP_071740_1980 (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 | 17.68 | 336. | -2.7 | 14.17 | 51.3 | 49.1 |
| North Polar Residual Cap Topography: ESP_071638_2675 ESP_071798_2675 (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 | 87.52 | 194. | -8.4 | -27.3 | 66.8 | 69.6 |
| Danielson Crater Outcrops: ESP_071779_1880 ESP_071634_1880 (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 | 7.671 | 353. | 8.73 | -5.62 | 52.6 | 53.9 |
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