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.
Well Developed Hollows and Ridges in Nilosyrtis Region Crater: ESP_018144_2185 ESP_018856_2185 (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 | 37.98 | 75.6 | 6.46 | 17.99 | 42.1 | 45.1 |
Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater: ESP_018268_2335 ESP_033854_2335 (Interval in Earth days: 1215) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.34 | 289. | -4.9 | 20.21 | 46.1 | 47.4 |
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 |
Erosional Surface Features in Arabia Terra: ESP_018488_2120 ESP_019345_2120 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.70 | 46.1 | -5.1 | 17.79 | 44.8 | 48.9 |
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 |
Two Distinct Surfaces along Mesa Wall in Deuteronilus Mensae: ESP_018225_2275 ESP_018146_2275 (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 | 47.18 | 22.7 | 5.82 | -17.3 | 43.5 | 45.3 |
Cones at Edge of North Polar Layered Deposits: ESP_018295_2580 ESP_026985_2580 (Interval in Earth days: 677) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.99 | 263. | -6.6 | -21.3 | 57.3 | 57.6 |
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 |
Mass Wasting on Steep North-Polar Boundary Scarp: ESP_018115_2640 ESP_018932_2640 (Interval in Earth days: 63) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.82 | 121. | -0.2 | 13.54 | 59.8 | 65.3 |
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