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.
| 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 |
| 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 |
| 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 |
| 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 |
| Fresh 3-Kilometer Diameter Crater near Margaritifer Region: ESP_018398_1715 ESP_025690_1715 (Interval in Earth days: 568) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.64 | 347. | 5.56 | -4.83 | 59.0 | 53.7 |
| 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 |
| 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 |
| Bull's-Eye Impact Crater: ESP_018522_2270 ESP_019010_2270 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.56 | 194. | 2.26 | -21.5 | 45.4 | 51.7 |
| Future Mars Landing Site in Acidalia Mensa: ESP_018161_2270 ESP_018227_2270 (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 | 46.68 | 331. | -1.6 | -15.5 | 43.8 | 45.4 |
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