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.
| Fractured Source Region of Kasei Valles: ESP_027406_2020 ESP_027261_2020 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.79 | 295. | 4.55 | -14.6 | 45.0 | 46.1 |
| Rayed Crater in Hesperia Planum: ESP_027545_1530 ESP_027611_1530 (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 | -26.6 | 108. | -6.1 | -23.8 | 69.5 | 70.4 |
| Change Detection in North Polar Crater: ESP_027622_2645 ESP_027438_2645 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.33 | 120. | 7.12 | -8.45 | 64.4 | 63.4 |
| Possible Future Landing Site in Sabrina Vallis Outlet: ESP_027656_1920 ESP_027168_1920 (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 | 11.87 | 313. | -3.6 | 13.23 | 49.2 | 46.9 |
| Phyllosilicates in Libya Montes Region: ESP_027559_1845 ESP_027836_1845 (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 | 4.654 | 82.1 | -3.6 | -18.9 | 51.7 | 53.2 |
| Change Detection for North Polar Dunes: ESP_027530_2615 ESP_027345_2615 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.19 | 137. | -10. | 4.844 | 62.4 | 59.9 |
| North Polar Dunes Change Detection: ESP_027581_2615 ESP_027396_2615 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.31 | 182. | -6.6 | 8.148 | 62.7 | 60.2 |
| Candidate Future Landing Site North of Hellas Planitia: ESP_027481_1540 ESP_025714_1540 (Interval in Earth days: 137) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.8 | 54.6 | 3.40 | -6.59 | 68.7 | 65.5 |
| North Polar Gypsum Dune Changes: ESP_027436_2615 ESP_027462_2615 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 81.44 | 180. | -7.2 | 7.495 | 61.5 | 60.9 |
| Dune Migration: ESP_027738_2590 ESP_027646_2590 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.99 | 212. | 7.64 | -8.70 | 62.0 | 62.1 |
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