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.
| Secondary Craters in Bas Relief: ESP_049076_1845 ESP_049564_1845 (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 | 4.415 | 171. | 2.64 | -21.6 | 41.0 | 37.5 |
| A Sneak Peek into Saheki’s Secret Layers : ESP_049172_1585 ESP_049528_1585 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.4 | 73.1 | 7.60 | 23.93 | 30.2 | 28.4 |
| Sinuous Ridge in Tempe Terra : ESP_049573_2265 ESP_049639_2265 (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 | 46.18 | 276. | 5.88 | -6.78 | 66.1 | 65.6 |
| Small Crater on South Polar Layered Deposits : ESP_049637_0920 ESP_049860_0920 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.9 | 40.6 | 11.9 | 23.22 | 75.5 | 78.0 |
| Candidate Human Exploration Zone in Noachis Terra: ESP_049427_1600 ESP_085389_1600 (Interval in Earth days: 2802) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.6 | 311. | 6.48 | -16.8 | 29.6 | 39.2 |
| Small Channel on Floor of Larger Channel in Western Libya Montes: ESP_049620_1810 ESP_049976_1810 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.919 | 81.0 | 0.12 | 23.82 | 33.8 | 30.2 |
| Isolated Secondary Cluster from a Well-Preserved Crater in Hesperia Planum: ESP_049698_1540 ESP_049553_1540 (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 | -25.7 | 115. | -1.1 | -21.9 | 32.2 | 33.0 |
| Faults in Zephyria Planum : ESP_049446_1800 ESP_057424_1800 (Interval in Earth days: 621) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.01 | 151. | -1.1 | 27.25 | 34.8 | 42.2 |
| Viscous Crater Fill in Noachis Terra : ESP_049307_1415 ESP_058116_1415 (Interval in Earth days: 686) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.1 | 350. | -2.8 | 6.714 | 34.8 | 33.9 |
| Possible Pit in South Polar Layered Deposits : ESP_049339_0920 ESP_049206_0920 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -88.0 | 257. | 12.8 | 23.05 | 71.3 | 68.6 |
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