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.
| Glacier Layering Revealed by Impact Crater on Viscous Flow Features Surface: ESP_089764_2200 ESP_089487_2200 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.61 | 17.6 | -8.7 | 10.06 | 52.8 | 48.4 |
| Streamlined Shape and Possible Bar South of Semeykin Crater: ESP_089883_2195 ESP_090028_2195 (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 | 39.01 | 8.16 | -0.2 | 14.06 | 53.3 | 53.8 |
| Double Crater: ESP_089603_2125 ESP_089880_2125 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.26 | 93.1 | -1.8 | -20.5 | 49.9 | 54.1 |
| Kasei Valles Alluvial Fan and Distributary Channels: ESP_089899_2035 ESP_089622_2035 (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 | 23.09 | 293. | -4.0 | 17.28 | 52.5 | 48.8 |
| Debris Apron in Phlegra Montes: ESP_089864_2285 ESP_090009_2285 (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 | 47.97 | 165. | -0.6 | 11.32 | 55.2 | 56.1 |
| Enigmatic Ridges in Aeolis Region: ESP_089601_1800 ESP_089957_1800 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.00 | 151. | 6.59 | 22.31 | 55.7 | 54.6 |
| Lava Flows in Elysium Region: ESP_089640_1960 ESP_089996_1960 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.79 | 164. | 1.96 | 17.68 | 51.3 | 51.8 |
| Kasei Valles Alluvial Fans and Flood Terrace: ESP_089820_2025 ESP_089675_2025 (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 | 22.03 | 290. | -0.2 | -16.9 | 51.7 | 52.1 |
| Crater in Arabia Terra: ESP_089804_2205 ESP_090160_2205 (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 | 39.96 | 7.23 | -21. | -7.62 | 54.5 | 57.6 |
| Hillslope Morphologies in Roddy Crater: ESP_089885_1585 ESP_090030_1585 (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 | -21.1 | 320. | 5.83 | 24.57 | 64.9 | 62.7 |
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