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.
| Valley Breaching Gale Crater Rim: ESP_071642_1735 ESP_071787_1735 (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 | -6.40 | 136. | -8.6 | 6.598 | 60.5 | 58.9 |
| 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 |
| Scallop-Hosting Mantle in Utopia Planitia: ESP_071881_2265 ESP_071815_2265 (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 | 46.29 | 82.6 | 3.99 | 19.89 | 50.4 | 48.3 |
| 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 |
| Flow Feature near Huo Hsing Vallis: ESP_071618_2100 ESP_071829_2100 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 29.67 | 66.7 | -0.7 | -11.3 | 48.1 | 49.8 |
| 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 |
| Channel in Bedrock: ESP_071819_1870 ESP_072254_1870 (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 | 7.021 | 341. | 5.67 | 27.87 | 53.1 | 52.1 |
| Dune-Ice Topography in Olympia Undae: ESP_071875_2615 ESP_071545_2615 (Interval in Earth days: 25) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.60 | 229. | -2.1 | 13.94 | 65.2 | 61.1 |
| Layers in Meridiani Planum: ESP_071647_1865 ESP_071792_1865 (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 | 6.317 | 358. | -7.7 | 6.1 | 54.6 | 53.3 |
| Lines of Pits in Protonilus Mensae: ESP_070735_2240 ESP_071869_2240 (Interval in Earth days: 88) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 43.59 | 52.3 | 5.50 | -8 | 45.8 | 50.8 |
Page 166 of 881 (8,805 images) | |||||