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.
| Possible Olivine-Rich Terrain: ESP_016903_1820 ESP_018248_1820 (Interval in Earth days: 105) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.941 | 123. | 0.64 | -15.9 | 48.8 | 54.5 |
| Filled Crater in Amazonis Planitia at End of Marte Vallis: ESP_017032_2050 ESP_018100_2050 (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 | 24.66 | 198. | -5.6 | 7.91 | 42.0 | 43.4 |
| Possible Phyllosilicates in Davies Crater: ESP_016960_2265 ESP_017949_2265 (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 | 45.96 | 0.18 | 5.68 | -8.98 | 42.3 | 43.7 |
| Possible Sulfate Mound in Juventae Chasma: ESP_016923_1755 ESP_086207_1755 (Interval in Earth days: 5398) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.26 | 297. | 0 | -13.1 | 52.4 | 42.7 |
| Aeolian Scour Features: ESP_017257_1680 ESP_017758_1680 (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 | -11.6 | 180. | -12. | 7.325 | 59.8 | 60.5 |
| Mesa in Chaos Terrain: ESP_017133_1810 ESP_017344_1810 (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 | 1.091 | 323. | 4.85 | -4.9 | 50.4 | 52.1 |
| Crater with Gullies in Acidalia Planitia: ESP_017080_2285 ESP_017502_2285 (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 | 47.90 | 323. | 4.87 | -6.70 | 42.6 | 43.2 |
| Rayed Crater West of Granicus Valles: ESP_017048_2040 ESP_017193_2040 (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 | 23.93 | 122. | -7.9 | 4.286 | 42.4 | 41.7 |
| Well-Preserved 15-Kilometer Impact Crater Northwest of Hellas Planitia: ESP_016958_1550 ESP_017736_1550 (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 | -24.6 | 64.4 | 4.47 | -9.81 | 65.7 | 70.5 |
| Bedrock Exposures in Northwest Coprates Chasma: ESP_016976_1705 ESP_017187_1705 (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 | -9.54 | 290. | 10.2 | -0.26 | 55.3 | 57.3 |
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