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.
| Very Fresh Small Crater : ESP_052794_1545 ESP_053572_1545 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.2 | 187. | 5.54 | -13.8 | 67.3 | 69.0 |
| Bright Mesas and Plains : ESP_052539_2360 ESP_052763_2360 (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 | 55.43 | 300. | -7.6 | 16.12 | 44.1 | 41.8 |
| Slope Monitoring : ESP_052582_2310 ESP_053004_2310 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.57 | 206. | -3.6 | -17.6 | 41.8 | 43.1 |
| Floor of Crater in Navua Valles : ESP_052666_1460 ESP_052877_1460 (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 | -33.8 | 81.1 | 27.5 | 18.10 | 72.0 | 73.4 |
| Zunil Crater Secondary Craters : ESP_052452_1940 ESP_052518_1940 (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 | 13.84 | 160. | 1.57 | -21.5 | 42.4 | 44.5 |
| Chains of Mounds in Utopia Planitia : ESP_052771_2125 ESP_053061_2125 (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 | 32.14 | 87.5 | 8.91 | 26.31 | 38.3 | 37.2 |
| Crater and Flow Near Galaxias Fluctus : ESP_052334_2135 ESP_052980_2135 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.18 | 139. | 7.81 | 22.94 | 37.8 | 37.3 |
| Banded or Terraced Hillslopes in East Hellas Planitia : ESP_052231_1410 ESP_060974_1410 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.5 | 82.4 | -4.9 | 20.53 | 74.5 | 73.0 |
| Megabreccia at Contact in Northeast Syrtis Major Region : ESP_052165_1975 ESP_052231_1975 (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 | 17.33 | 76.6 | 1.19 | -20.9 | 40.0 | 42.1 |
| Twin Channels in Innsbruck Crater : ESP_052143_1735 ESP_052565_1735 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.49 | 320. | -0.5 | -26.3 | 50.9 | 55.5 |
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