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.
| Well-Preserved Impact Crater: ESP_065749_1375 ESP_065195_1375 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -41.9 | 46.3 | -2.8 | 7.31 | 47.3 | 54.2 |
| Boundary of Ophir Chasma and Candor Chasma: ESP_065951_1750 ESP_066017_1750 (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 | -4.74 | 287. | 7.75 | -6.57 | 50.0 | 50.3 |
| Terrain Sample: ESP_065892_1370 ESP_066024_1370 (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 | -42.7 | 102. | 7.30 | -14.7 | 45.0 | 45.3 |
| Gully Monitoring and Topography: ESP_065744_1410 ESP_065876_1410 (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 | -38.6 | 181. | 2.17 | -22.2 | 46.5 | 46.8 |
| Layering in Crater West of Arabia Terra: ESP_065856_1890 ESP_066067_1890 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.762 | 358. | 4.30 | 24.27 | 57.8 | 54.8 |
| Gullies in Southern Hemisphere Crater: ESP_065915_1410 ESP_066047_1410 (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 | -38.8 | 195. | -7.9 | -28.7 | 45.3 | 45.6 |
| Cerberus Palus Lava: ESP_066088_1850 ESP_065191_1850 (Interval in Earth days: 70) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.786 | 148. | 1.92 | 21.46 | 53.8 | 57.3 |
| Bisected Polygonal Bedrock: ESP_065918_1935 ESP_083234_1935 (Interval in Earth days: 1349) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 13.13 | 106. | -3.5 | 4.659 | 60.4 | 61.0 |
| Layering in Crater: ESP_065840_1220 ESP_065972_1220 (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 | -57.4 | 84.6 | 7.60 | -9.28 | 49.8 | 49.7 |
| Fans and Polygons: ESP_065786_0925 ESP_065866_0925 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.2 | 167. | 8.69 | 2.249 | 66.3 | 66.8 |
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