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.
| Dunes and Sheets in Crater in Arabia Terra: ESP_080179_1910 ESP_080535_1910 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.67 | 352. | -5.0 | 20.04 | 52.8 | 51.6 |
| Dune Interaction with Residual Polar Ice: ESP_080175_2590 ESP_080623_2590 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.01 | 81.9 | 1.22 | 20.21 | 58.8 | 61.7 |
| North Polar Residual Cap: ESP_080027_2685 ESP_072140_2685 (Interval in Earth days: 615) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.45 | 183. | -27. | -19.8 | 65.4 | 73.7 |
| Mound in Chryse Planitia: ESP_080180_2060 ESP_080246_2060 (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 | 25.58 | 322. | 8.26 | -8.22 | 47.2 | 48.9 |
| Valleys along Lower Wallrock Slopes in Juventae Chasma: ESP_079825_1760 ESP_080313_1760 (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 | -4.19 | 297. | -2.1 | -14.2 | 59.4 | 60.5 |
| Layered Late-Stage Fan in Gale Crater: ESP_080187_1755 ESP_080332_1755 (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 | -4.26 | 137. | -23. | 0.545 | 61.2 | 59.5 |
| Steep Polar Scarp and Dune Source in Western Olympia Cavi: ESP_080081_2635 ESP_080186_2635 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.61 | 119. | -2.0 | 11.78 | 61.1 | 61.1 |
| Dune Interaction with Residual Polar Ice: ESP_079963_2615 ESP_080411_2615 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.45 | 104. | 1.18 | 16.81 | 59.0 | 61.2 |
| Moreux Crater Dunes: ESP_079900_2225 ESP_080045_2225 (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 | 42.16 | 44.3 | -3.2 | 12.11 | 45.6 | 44.9 |
| North Polar Residual Cap Topography: ESP_079914_2695 ESP_079678_2695 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 89.39 | 308. | -20. | -22.6 | 65.0 | 64.3 |
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