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.
Bedrock Exposures in Uzboi Vallis and a Crater Rim: ESP_013586_1490 ESP_021722_1490 (Interval in Earth days: 634) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.8 | 323. | -0.0 | -28.7 | 36.4 | 44.3 |
Small Rayed Crater in Syrtis Major Planum: ESP_012791_1910 ESP_012857_1910 (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 | 10.67 | 62.2 | 4.22 | -17.8 | 58.5 | 59.5 |
Gullies in Southern Hemisphere Crater: ESP_013894_1410 ESP_022676_1410 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.8 | 195. | -5.6 | 5.235 | 37.6 | 35.2 |
Layered Material Exposed on Crater Floor: ESP_013017_2150 ESP_013518_2150 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.69 | 8.85 | 6.51 | 22.48 | 72.6 | 67.8 |
Recent 10 Kilometer Diameter Crater in Ares Vallis: ESP_013335_1975 ESP_020772_1975 (Interval in Earth days: 580) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.40 | 329. | 1.40 | 17.37 | 58.3 | 58.8 |
Floor of Athabasca Valles: ESP_013526_1895 ESP_013671_1895 (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 | 9.610 | 156. | -3.5 | 12.84 | 51.2 | 48.4 |
Strike Slip Fault in Amazonis Planitia: ESP_012799_1990 ESP_013076_1990 (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 | 18.75 | 203. | 1.92 | -21.6 | 63.2 | 63.0 |
Possible Arete in North and South Debris Flows: ESP_013528_1380 ESP_013673_1380 (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 | -41.6 | 108. | -4.1 | 9.479 | 39.1 | 37.6 |
Ganges Mensa Layered Deposits: ESP_012993_1725 ESP_013059_1725 (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 | -7.39 | 310. | -5.5 | -26.0 | 48.5 | 49.3 |
Unusual Dune Form along Inner Small Crater Rim: ESP_013909_1145 ESP_014041_1145 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -65.1 | 151. | -0.4 | -20.7 | 51.9 | 54.5 |
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