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.
Cones at Edge of North Polar Layered Deposits: ESP_018333_2605 ESP_018926_2605 (Interval in Earth days: 46) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.20 | 295. | 6.93 | 22.29 | 58.1 | 62.3 |
Steep North-Polar Boundary Scarp: ESP_018190_2640 ESP_018941_2640 (Interval in Earth days: 59) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.01 | 230. | 1.83 | 15.95 | 60.1 | 65.4 |
High-Latitude Exposure of North Polar Layered Deposits: ESP_018380_2680 ESP_018605_2680 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.84 | 70.4 | -12. | -20.4 | 64.4 | 66.3 |
Fresh and Well-Preserved 20-Kilometer Diameter Impact Crater in Arabia Terr: ESP_018252_1965 ESP_018753_1965 (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 | 16.47 | 11.5 | -8.4 | 14.84 | 47.5 | 46.9 |
Layered Terrain in Aeolis Planum: ESP_018181_1730 ESP_018893_1730 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.83 | 152. | -5.0 | 11.41 | 58.6 | 56.8 |
Valley in Libya Montes: ESP_018223_1830 ESP_018368_1830 (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 | 2.730 | 84.7 | -6.4 | 9.665 | 53.4 | 52.3 |
Candor Chasma: ESP_018387_1730 ESP_019666_1730 (Interval in Earth days: 99) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.02 | 288. | -4.5 | 13.11 | 58.7 | 55.3 |
Light-Toned Outcrops in Noctis Region: ESP_018124_1720 ESP_018757_1720 (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 | -8.00 | 268. | 0.79 | -20.5 | 59.0 | 59.9 |
Central Structure of Wahoo Crater: ESP_018214_2035 ESP_018847_2035 (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 | 23.26 | 326. | 10.4 | -8.96 | 43.9 | 47.8 |
Longitudinally Aligned Cones: ESP_018457_2065 ESP_018747_2065 (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 | 26.25 | 173. | -8.5 | 18.07 | 45.6 | 44.5 |
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