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 |
| Possible Prehnite-Bearing Deposits in Northwest Hellas Planitia: ESP_027903_1535 ESP_026571_1535 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.2 | 56.1 | -7.1 | 12.83 | 67.6 | 69.4 |
| 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 |
| Ceraunius Fossae: ESP_028001_2070 ESP_053688_2070 (Interval in Earth days: 2001) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.57 | 253. | 5.82 | -5.11 | 47.6 | 42.7 |
| 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 |
| Mounds and Small Ridges along Wrinkle Ridge on Huygens Crater Floor: ESP_027969_1635 ESP_028325_1635 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.2 | 54.6 | -23. | -4.61 | 62.8 | 60.0 |
| Fretted Terrain Valley in Viking 084A73 and MOC SP2-45006: ESP_027889_2140 ESP_036394_2140 (Interval in Earth days: 663) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.72 | 70.1 | -2.1 | 11.65 | 47.6 | 45.5 |
| Extensive Outcrops of Rhythmic Stratigraphy in Arabia Terra: ESP_027918_1905 ESP_027984_1905 (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 | 10.30 | 1.23 | 3.76 | -15.5 | 49.8 | 51.5 |
| Terraced Lower Walls of Crater: ESP_027965_1890 ESP_088058_1890 (Interval in Earth days: 4682) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.001 | 158. | -1.7 | 8.505 | 50.7 | 49.3 |
| IR-Distinct Crater in Utopia Planitia: ESP_027941_2295 ESP_033110_2295 (Interval in Earth days: 403) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.18 | 88.4 | -2.7 | -19.2 | 51.3 | 54.5 |
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