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.
| Layering in Western Arabia Terra: ESP_067083_1895 ESP_067967_1895 (Interval in Earth days: 69) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.349 | 354. | -7.2 | 11.32 | 46.6 | 41.2 |
| Flow Features near Crater South of Burton Crater: ESP_067115_1640 ESP_067656_1640 (Interval in Earth days: 42) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.8 | 203. | 6.28 | -5.23 | 37.2 | 40.3 |
| Inverted Channel Feature: ESP_067281_1910 ESP_067492_1910 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.84 | 352. | -7.8 | 25.81 | 45.7 | 41.8 |
| Surface Features in Hellas Planitia: ESP_067279_1480 ESP_067345_1480 (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 | -31.4 | 50.9 | 6.46 | -2.66 | 40.1 | 41.3 |
| Large New Impact Crater: ESP_066951_2150 ESP_084385_2150 (Interval in Earth days: 1358) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.67 | 352. | -1.0 | 24.80 | 64.3 | 64.4 |
| Valley Channel in Central Arabia Terra: ESP_067147_2080 ESP_084660_2080 (Interval in Earth days: 1365) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 27.73 | 44.9 | 6.21 | 22.84 | 56.4 | 55.4 |
| Crater Rim and Ejecta Blanket: ESP_067222_1470 ESP_067829_1470 (Interval in Earth days: 47) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.8 | 167. | -4.0 | -16.4 | 40.7 | 48.9 |
| Shallow Channels Entering Collapse Terrain near Orson Welles Crater: ESP_066979_1780 ESP_073877_1780 (Interval in Earth days: 537) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.90 | 313. | -5.2 | 10.09 | 42.0 | 55.8 |
| Valleys in Crater Northeast of Argyre Region: ESP_067229_1500 ESP_067361_1500 (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 | -29.7 | 334. | 7.83 | -10.6 | 39.0 | 41.4 |
| Nilosyrtis Region Crater with Asymmetric Walls: ESP_066961_2100 ESP_075481_2100 (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 | 29.92 | 79.6 | 9.00 | -8.7 | 60.1 | 63.5 |
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