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.
| Yardangs in Aeolis Region: ESP_082204_1800 ESP_082336_1800 (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 | -0.07 | 151. | 6.30 | -25.1 | 57.9 | 60.5 |
| Lava Interactions with Landscape: ESP_082228_1545 ESP_082663_1545 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.2 | 221. | -7.6 | 21.04 | 60.0 | 53.2 |
| Chryse Chaos: ESP_082290_1885 ESP_082356_1885 (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 | 8.575 | 323. | 8.00 | -7.61 | 59.2 | 60.6 |
| Cones: ESP_082416_2015 ESP_082139_2015 (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 | 21.13 | 123. | -4.7 | 6.682 | 64.5 | 61.5 |
| Ridges in Meridiani Planum: ESP_082289_1805 ESP_082355_1805 (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 | 0.516 | 351. | 8.46 | -7.68 | 57.8 | 59.0 |
| Lava-Coated Crater near Kasei Valles: ESP_082265_1960 ESP_082555_1960 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 15.66 | 285. | 1.99 | 21.45 | 61.3 | 61.1 |
| Volcanic Vent East of Pavonis Mons: ESP_082174_1795 ESP_082240_1795 (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 | -0.46 | 251. | -3.3 | -20.3 | 58.6 | 60.0 |
| Hillslope Morphologies in Crater: ESP_082342_1655 ESP_090372_1655 (Interval in Earth days: 626) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.4 | 347. | 3.30 | -13.1 | 57.2 | 61.3 |
| Lava-Topography Interactions: ESP_082294_1535 ESP_082162_1535 (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 | -26.4 | 221. | -23. | 8.101 | 60.8 | 59.7 |
| Partly-Filled Impact Crater near Nicholson Crater: ESP_082176_1830 ESP_082242_1830 (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 | 2.848 | 196. | -7.6 | -23.2 | 59.3 | 60.7 |
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