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.
| Streamlined Landforms in Tinjar Valles: ESP_025988_2165 ESP_026067_2165 (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 | 36.37 | 126. | -2.8 | 24.21 | 40.1 | 37.7 |
| Field of Transverse Aeolian Ridges with Superposed Impact Craters: ESP_025966_1765 ESP_026889_1765 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.32 | 12.8 | -16. | 0.66 | 53.2 | 55.2 |
| Well-Preserved Impact Crater on Northern Plains: ESP_025971_2350 ESP_026103_2350 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.46 | 225. | 8.64 | -15.0 | 43.4 | 45.1 |
| Interior Deposits of Pangboche Crater: ESP_026024_1975 ESP_026169_1975 (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 | 17.25 | 226. | -13. | 1.589 | 43.7 | 43.1 |
| Eastern Rim of Well-Preserved 15-Kilometer Crater Near Alba Mons: ESP_026142_2195 ESP_025852_2195 (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 | 39.10 | 238. | 17.9 | -3.88 | 38.6 | 40.4 |
| Fresh 4-Kilometer Crater South of Isidis Planitia: ESP_025950_1755 ESP_025805_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 | -4.27 | 86.5 | 23.9 | 7.715 | 51.0 | 51.2 |
| Channel and Fan System in Reuyl Crater: ESP_026079_1700 ESP_026224_1700 (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 | -10.0 | 167. | -0.1 | 15.48 | 56.9 | 56.7 |
| Well-Preserved Impact Crater in Utopia Planitia: ESP_026015_2045 ESP_026292_2045 (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 | 24.43 | 107. | 27.8 | 4.068 | 38.2 | 41.2 |
| Intersection of Ridges in Pavonis Mons: ESP_025997_1850 ESP_026630_1850 (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 | 4.788 | 244. | 0 | -19.2 | 47.9 | 51.6 |
| Flow Features in Crater Near Cerberus Fossae: ESP_025934_1905 ESP_026567_1905 (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 | 10.41 | 162. | 6.71 | -13.0 | 44.4 | 48.3 |
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