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.
| 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 |
| Deflected Ejecta of Arabia Region Crater: ESP_017356_2175 ESP_024872_2175 (Interval in Earth days: 586) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.02 | 350. | 0 | 20.49 | 41.2 | 39.9 |
| Possible Clay Beds in West Ladon Valles Channels: ESP_017489_1610 ESP_035119_1610 (Interval in Earth days: 1374) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.9 | 326. | -5.8 | -19.4 | 65.4 | 66.3 |
| Terraced Pedestal Crater in CTX Image: ESP_017497_2325 ESP_017774_2325 (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 | 52.23 | 97.6 | 3.87 | -14.3 | 43.3 | 45.0 |
| Crater Cut by Horst and Graben: ESP_017399_2185 ESP_017900_2185 (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 | 38.10 | 256. | -4.2 | 10.29 | 41.5 | 41.1 |
| Circular Features in Far Northern Reaches of Arcadia Planitia: ESP_017632_2475 ESP_018634_2475 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.05 | 9.22 | -2.5 | 13.14 | 49.8 | 52.6 |
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