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 on Northern Plains: ESP_017373_2350 ESP_016740_2350 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.59 | 245. | -13. | 0 | 45.6 | 46.6 |
| Candidate MSL Landing Site in Northeast Syrtis Major: ESP_017498_1980 ESP_018566_1980 (Interval in Earth days: 84) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.52 | 76.9 | -8.1 | 12.23 | 45.4 | 46.2 |
| Nili Patera Caldera and Dunes: ESP_017617_1890 ESP_034891_1890 (Interval in Earth days: 1346) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.020 | 67.5 | 9.95 | -9.19 | 47.9 | 48.1 |
| Northern Plains Craters: ESP_017386_2315 ESP_018019_2315 (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 | 51.23 | 248. | 1.71 | -13.4 | 43.3 | 45.2 |
| Light-Toned Layering in Noctis Region Pit: ESP_017399_1680 ESP_027236_1680 (Interval in Earth days: 766) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.8 | 263. | -4.9 | -24.5 | 60.2 | 62.0 |
| Central Peaks of Two Impact Craters: ESP_017437_1550 ESP_017859_1550 (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 | -24.9 | 306. | 9.49 | -8.80 | 68.6 | 70.7 |
| Young Esker-Like Ridges in Tempe Terra: ESP_017477_2190 ESP_018545_2190 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.42 | 287. | -6.9 | 8.883 | 41.9 | 43.8 |
| Pits on Fan Surfaces in Mojave Crater: ESP_017568_1870 ESP_018069_1870 (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 | 7.120 | 326. | -6.1 | 13.95 | 49.9 | 49.5 |
| Valley Crossing Mare-Type Ridge in Solis Planum: ESP_017425_1565 ESP_017926_1565 (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 | -23.1 | 274. | -3.0 | 16.24 | 67.9 | 68.1 |
| Degrading Craters on Northern Plains: ESP_017308_2315 ESP_017598_2315 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.90 | 220. | -9.0 | 6.936 | 44.2 | 42.7 |
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