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.
| Exposure of Mid-Latitude Apron Interior by Younger Gully: ESP_015947_1370 ESP_051036_1370 (Interval in Earth days: 2734) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -42.5 | 308. | -3.0 | -16.8 | 66.5 | 62.9 |
| Central Peak of an Impact Crater in Terra Sabaea: ESP_016153_1565 ESP_020188_1565 (Interval in Earth days: 314) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.0 | 81.0 | 7.63 | -4.44 | 55.4 | 59.1 |
| Layered Material Seen in MOC Image M0807392 in Focas Crater: ESP_016208_2135 ESP_017975_2135 (Interval in Earth days: 138) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.42 | 12.7 | 1.67 | -15.9 | 41.0 | 43.8 |
| Sulfate Layered Stratigraphy in Ophir Region: ESP_015974_1760 ESP_020220_1760 (Interval in Earth days: 331) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.85 | 285. | 4.82 | -15.3 | 43.0 | 56.3 |
| Layer Exposure in Crater North of Meridiani Planum: ESP_015958_1835 ESP_016235_1835 (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 | 3.571 | 1.15 | 11.6 | -17.7 | 39.8 | 44.4 |
| Large Polygons: ESP_016098_1415 ESP_016164_1415 (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 | -38.1 | 144. | 7.55 | -11.8 | 64.9 | 66.9 |
| Possible MSL Landing Site in Mawrth Vallis: ESP_015985_2040 ESP_016262_2040 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.82 | 341. | 13.7 | -11.8 | 38.3 | 40.8 |
| Crater Rim Gullies Filled with Small Dunes: ESP_015934_2165 ESP_037243_2165 (Interval in Earth days: 1660) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.09 | 292. | 1.58 | -16.4 | 42.8 | 56.6 |
| Light-Toned Material on Plateau North of Aurorae Chaos: ESP_016157_1745 ESP_016790_1745 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.39 | 330. | -6.7 | -21.1 | 46.4 | 53.5 |
| Distinct Spur and Gully Mesa in Candor Chasma: ESP_016185_1740 ESP_016330_1740 (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 | -6.09 | 285. | 8.13 | 23.94 | 46.0 | 46.4 |
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