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 |
Cones at Edge of North Polar Layered Deposits: ESP_018387_2600 ESP_026576_2600 (Interval in Earth days: 638) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.99 | 270. | -8.4 | -24.5 | 59.2 | 58.2 |
Layered Terrain in Aeolis and Zephyria Regions: ESP_018392_1740 ESP_018814_1740 (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 | -5.89 | 150. | 6.24 | -8.79 | 57.3 | 57.9 |
Well-Preserved 5-Kilometer Diameter Impact Crater: ESP_018478_2150 ESP_018979_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 | 34.78 | 318. | -3.5 | 13.05 | 44.5 | 46.3 |
Light-Toned Outcrops in Noctis Region: ESP_018480_1725 ESP_024994_1725 (Interval in Earth days: 508) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.30 | 268. | 7.71 | -7.73 | 58.0 | 46.2 |
Cones at Edge of North Polar Layered Deposits: ESP_018109_2580 ESP_026654_2580 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.90 | 298. | -0.4 | -19.2 | 56.1 | 56.6 |
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 |
Rounded Mounds in Cydonia Region: ESP_018411_2235 ESP_018134_2235 (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 | 43.13 | 346. | -1.5 | 17.83 | 44.5 | 41.4 |
Columbus Crater: ESP_018351_1510 ESP_018496_1510 (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 | -28.7 | 194. | -7.0 | 8.364 | 73.0 | 71.7 |
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 |
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