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.
| Layering in Crater West of Arabia Terra: ESP_065856_1890 ESP_066067_1890 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.762 | 358. | 4.30 | 24.27 | 57.8 | 54.8 |
| Ridges along Pavonis Mons Caldera Rim: ESP_065992_1810 ESP_073853_1810 (Interval in Earth days: 612) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.999 | 248. | 6.46 | 17.64 | 52.4 | 56.1 |
| Landforms South of Isidis Planitia: ESP_066024_1820 ESP_075019_1820 (Interval in Earth days: 700) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.779 | 94.9 | 3.53 | -7.12 | 52.7 | 50.0 |
| Mesa in Low Northern Latitudes: ESP_066046_1900 ESP_073973_1900 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.890 | 213. | 2.52 | -8.89 | 57.1 | 61.0 |
| Slope Failures in Tempe Terra: ESP_065925_2175 ESP_066057_2175 (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 | 37.31 | 273. | -9.9 | -28.1 | 76.5 | 77.1 |
| Pit in Mid-Latitude Deposit: ESP_065905_1315 ESP_066591_1315 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.3 | 109. | 1.16 | -13.6 | 46.5 | 44.1 |
| Valley Cutting Ejecta of Crater and Associated Sinuous Ridge: ESP_065902_1685 ESP_065968_1685 (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 | -11.3 | 185. | 7.46 | -6.99 | 47.9 | 48.2 |
| Aram Chaos: ESP_066015_1815 ESP_065804_1815 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.686 | 339. | 12.8 | -7.98 | 52.1 | 55.4 |
| Gully Monitoring and Topography: ESP_065744_1410 ESP_065876_1410 (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 | -38.6 | 181. | 2.17 | -22.2 | 46.5 | 46.8 |
| Terrain Sample: ESP_065892_1370 ESP_066024_1370 (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 | -42.7 | 102. | 7.30 | -14.7 | 45.0 | 45.3 |
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