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.
| Utopia Planitia: ESP_071089_2050 ESP_071722_2050 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.63 | 110. | 1.86 | -21.6 | 48.2 | 50.8 |
| Active Dune Monitoring in Meridiani Planum: ESP_071080_1840 ESP_071014_1840 (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 | 3.976 | -0.8 | -7.0 | 17.06 | 56.7 | 55.0 |
| West Flank of Chasma Boreale Barchan and Linear Dunes: ESP_070975_2645 ESP_071014_2645 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.20 | 323. | -8.5 | 6.328 | 60.8 | 60.1 |
| Inverted Channels and Clay-Rich Terrain in Mawrth Vallis: ESP_071041_2060 ESP_070975_2060 (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 | 25.90 | 341. | -7.8 | 12.98 | 48.7 | 47.0 |
| Equatorial-Facing Trough Exposure of North Polar Layered Deposits: ESP_070981_2665 ESP_070982_2665 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.41 | 128. | 2.59 | -12.2 | 61.7 | 62.3 |
| Dark Slope Streaks in Arabia Terra: ESP_070986_1945 ESP_070841_1945 (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 | 14.23 | 44.4 | -7.4 | -18.7 | 52.3 | 53.3 |
| Mawrth Vallis Stratigraphy: ESP_070896_2015 ESP_070474_2015 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.24 | 341. | -12. | 11.29 | 50.4 | 48.7 |
| Snowy Dunes: ESP_070934_2560 ESP_071092_2560 (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 | 75.59 | 13.4 | -8.8 | 6.901 | 56.3 | 55.6 |
| Possible Layers in Korolev Crater: ESP_071047_2535 ESP_071034_2535 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 73.14 | 163. | 8.1 | -7.01 | 54.1 | 55.3 |
| Well-Preserved Mid-Latitude Impact Crater: ESP_070881_2205 ESP_070815_2205 (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 | 40.21 | 27.1 | 1.09 | 17.77 | 46.2 | 44.6 |
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