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.
| Gullies in Dunes: ESP_014151_1325 ESP_021509_1325 (Interval in Earth days: 573) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.1 | 19.5 | 5.65 | -10.1 | 42.1 | 48.1 |
| Gullies on Southwest Slope of Asimov Crater: ESP_012767_1320 ESP_012912_1320 (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 | -47.5 | 4.40 | 10.5 | 21.65 | 47.2 | 44.3 |
| Possible Rootless Cones in Hydraotes Chaos: ESP_013177_1800 ESP_021458_1800 (Interval in Earth days: 645) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.053 | 326. | -4.9 | -21.2 | 49.8 | 53.9 |
| Stratigraphy of Possible Sulfate and Zeolite at Mawrth Vallis: ESP_013229_2050 ESP_013295_2050 (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 | 24.51 | 341. | 14.8 | -5.47 | 63.5 | 64.0 |
| Gullies in Southern Hemisphere Crater: ESP_013894_1410 ESP_022676_1410 (Interval in Earth days: 684) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.8 | 195. | -5.6 | 5.235 | 37.6 | 35.2 |
| Lineated Valley Fill in Nilosyrtis Mensae: ESP_014162_2135 ESP_020597_2135 (Interval in Earth days: 501) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 33.08 | 68.5 | 6.58 | -16.0 | 59.0 | 66.6 |
| Flood Lava Passing through a Constriction in Amazonis Planitia: ESP_014184_2070 ESP_020276_2070 (Interval in Earth days: 475) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.88 | 190. | -8.6 | 13.66 | 54.9 | 58.4 |
| Excellent Exposure of Layered Mound in Terby Crater: ESP_013872_1520 ESP_014017_1520 (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 | -27.5 | 74.3 | 1.04 | 15.03 | 34.6 | 33.2 |
| Gullies Oriented around Large Obstacle in MOC Image E1002766: ESP_014132_1425 ESP_020791_1425 (Interval in Earth days: 519) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.2 | 178. | -8.6 | 14.15 | 38.0 | 54.6 |
| Fresh Central Pit Crater in Southern Highlands: ESP_012727_1540 ESP_013149_1540 (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 | -25.8 | 14.6 | -3.1 | -14.1 | 46.9 | 42.2 |
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