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.
| North Polar Gypsum Dune Changes: ESP_027898_2620 ESP_027661_2620 (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 | 81.79 | 158. | 7.13 | -7.81 | 65.8 | 63.9 |
| Pitted Northern Plains: ESP_027919_2215 ESP_028064_2215 (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 | 41.11 | 332. | -18. | -4.69 | 50.4 | 50.8 |
| Fan of Overlapping Curvilinear Ridges in Saheki Crater: ESP_028021_1580 ESP_028865_1580 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.8 | 73.2 | 6.27 | -5.89 | 63.6 | 59.3 |
| Colorful Surface near Nili Fossae: ESP_019753_2000 ESP_019898_2000 (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 | 19.72 | 72.4 | -16. | -0.39 | 54.6 | 54.4 |
| Exploring the Mounds in the Chryse Region: ESP_027339_2060 ESP_026284_2060 (Interval in Earth days: 82) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.96 | 326. | -16. | -3.07 | 45.8 | 41.5 |
| A Crater North of Coprates Chasma: ESP_027775_1675 ESP_028052_1675 (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 | -12.4 | 307. | 8.65 | -9.17 | 59.1 | 59.5 |
| Nested Craters: ESP_027610_2205 ESP_042801_2205 (Interval in Earth days: 1184) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.10 | 125. | -0.8 | -21.0 | 45.8 | 43.9 |
| Candidate Future Landing Site Near Mawrth Vallis: ESP_027444_2065 ESP_026745_2065 (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 | 25.98 | 339. | -8.4 | 12.67 | 45.5 | 41.3 |
| 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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