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.
| Western Slope of Asimov Crater: ESP_013110_1325 ESP_013611_1325 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.0 | 4.17 | -23. | -7.91 | 45.4 | 41.0 |
| Upper Reach of Mamers Valles: ESP_013254_2115 ESP_021825_2115 (Interval in Earth days: 668) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.09 | 18.9 | 5.76 | 15.24 | 68.5 | 68.2 |
| Marte Vallis Streamlined Landforms: ESP_014092_1955 ESP_014158_1955 (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 | 15.46 | 183. | -6.8 | -25.9 | 48.1 | 48.6 |
| Possible Clay and Sulfate in Terra Sirenum Layered Deposit: ESP_013485_1535 ESP_013907_1535 (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 | -26.0 | 199. | 4.43 | -12.0 | 36.9 | 35.3 |
| Light-Toned Material in a Crater in Iani Chaos: ESP_013572_1795 ESP_022710_1795 (Interval in Earth days: 712) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.54 | 341. | -3.2 | 13.82 | 44.7 | 37.9 |
| Mawrth Region Stratigraphy in Crater Wall: ESP_013651_2045 ESP_014284_2045 (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 | 24.04 | 342. | -2.1 | -22.0 | 59.6 | 52.4 |
| Trough in Phoenicis Lacus: ESP_013971_1675 ESP_014327_1675 (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 | -12.2 | 249. | -2.9 | 9.647 | 35.6 | 32.9 |
| Well-Preserved Crater with Central Peak in Chryse Planitia: ESP_013810_2085 ESP_022869_2085 (Interval in Earth days: 706) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.43 | 319. | 5.59 | -12.7 | 60.4 | 56.9 |
| Candidate Landing Site in Terra Sabaea and Tyrrhenna Terra Boundary: ESP_013925_1580 ESP_014426_1580 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.7 | 66.6 | 0.50 | 25.72 | 34.3 | 32.1 |
| Floor of Athabasca Valles: ESP_013526_1895 ESP_013671_1895 (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 | 9.610 | 156. | -3.5 | 12.84 | 51.2 | 48.4 |
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