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.
| Crater with Debris Aprons in Tyrrhena Terra: ESP_031805_1545 ESP_031950_1545 (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 | -25.2 | 84.1 | 3.68 | 21.79 | 32.2 | 31.3 |
| Valleys in Tyrrhena Terra: ESP_031817_1410 ESP_031751_1410 (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 | -38.8 | 118. | 5.17 | 22.85 | 36.9 | 35.1 |
| Eastern Valles Marineris Bedrock Stratigraphy and Falling Dunes: PSP_010277_1650 PSP_010699_1650 (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 | -14.6 | 302. | -8.0 | -24.2 | 63.3 | 63.2 |
| Sedimentary Bedrock Diversity in Terby Crater: ESP_031212_1525 ESP_031278_1525 (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 | -27.1 | 73.9 | 17.1 | -4.75 | 33.2 | 34.5 |
| South Polar Layered Deposit Spiral Troughs during Katabatic Wind Season: ESP_031048_0945 ESP_031100_0945 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 289. | -13. | 2.826 | 65.5 | 64.1 |
| Well-Preserved Crater in Hesperia Planum: ESP_031171_1610 ESP_032160_1610 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.8 | 113. | 1.89 | -8.45 | 35.8 | 33.3 |
| USGS Dune Database 2280-788 Changes: ESP_031194_1010 ESP_031141_1010 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -78.7 | 228. | -14. | 3.468 | 60.1 | 58.8 |
| Monitor Steep Slopes in Depression North of Ganges Chasma: ESP_031032_1765 ESP_031177_1765 (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 | -2.61 | 308. | -19. | -3.73 | 45.0 | 42.3 |
| Sediments in Valleys Upslope of Ladon Valles Basin: ESP_030939_1600 ESP_031796_1600 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.9 | 327. | -2.4 | 17.48 | 38.4 | 30.6 |
| Reull Vallis Sample: ESP_031092_1425 ESP_031237_1425 (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 | -37.1 | 112. | 5.11 | 19.31 | 36.1 | 34.2 |
Page 512 of 878 (8,772 images) | |||||