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.
| Fresh Impact Crater: ESP_026661_1495 ESP_062977_1490 (Interval in Earth days: 2830) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -30.2 | 120. | 3.50 | -8.29 | 72.9 | 72.0 |
| Dunes and North Polar Outlier in MOC Image R23-00720: ESP_026607_2590 ESP_026910_2590 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 78.95 | 131. | -0.7 | 14.42 | 55.9 | 55.6 |
| Possible Future Landing Site Near Coprates Chasma: ESP_026615_1675 ESP_026338_1675 (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 | -12.6 | 296. | -21. | 5.341 | 62.1 | 59.5 |
| Central Peak of Ottumwa Crater: ESP_026931_2050 ESP_027709_2050 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.56 | 304. | -14. | 5.156 | 44.4 | 45.9 |
| Crater with Disrupted Interior and Channel Exiting South End: ESP_026709_2030 ESP_027408_2030 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.59 | 243. | 7.12 | -16.1 | 42.5 | 46.5 |
| Dry Cataracts in the Southern Branch of Kasei Valles: ESP_026918_2045 ESP_026430_2045 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.41 | 299. | -20. | 5.839 | 44.9 | 41.4 |
| Eroded Scarp Near Terminus of Valleys on Western Hecates Tholus: ESP_026752_2125 ESP_027029_2125 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.12 | 148. | -3.1 | -21.6 | 41.7 | 44.3 |
| Proposed Site for Future Exploration in Cerberus Palus: ESP_026950_1870 ESP_027016_1870 (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 | 6.777 | 146. | 0.08 | -20.2 | 49.8 | 51.5 |
| North Polar Linear Dune Changes: ESP_026942_2640 ESP_026692_2640 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.82 | 318. | 14.3 | 0.356 | 59.2 | 59.2 |
| IR-Distinct Crater: ESP_026619_2285 ESP_027107_2285 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.34 | 176. | 4.39 | -12.0 | 41.7 | 44.9 |
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