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.
| Noachis Region Clays: ESP_011592_1595 ESP_011658_1595 (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 | -20.3 | 40.3 | 4.94 | -17.2 | 58.3 | 59.6 |
| Distinctive Small Rayed Crater in Terra Cimmeria: PSP_010863_1720 ESP_020133_1720 (Interval in Earth days: 723) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.92 | 142. | -1.8 | -20.3 | 58.8 | 57.3 |
| Possible Chloride Salt Deposits Observed in THEMIS: PSP_010597_1470 PSP_007380_1470 (Interval in Earth days: 251) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.7 | 205. | 18.1 | -6.34 | 69.5 | 63.4 |
| Flow Feature in Southern Utopia Planitia: ESP_011497_1965 ESP_064454_1965 (Interval in Earth days: 4126) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.22 | 110. | -4.3 | -24.5 | 59.6 | 61.7 |
| High-Latitude Exposure of North Polar Layered Deposits: PSP_010808_2720 ESP_028150_2680 (Interval in Earth days: 1351) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.93 | 95.5 | -6.3 | -11.4 | 79.4 | 74.3 |
| Complex Morphology in Acidalia Region: ESP_011384_2185 ESP_011661_2185 (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 | 38.01 | 310. | 7.35 | -13.2 | 63.5 | 68.9 |
| Ithaca Region Plumes: ESP_011350_0945 ESP_011351_0945 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.2 | 181. | 22.8 | -3.81 | 87.6 | 89.8 |
| Very Fresh Unnamed Crater in Tyrrhena Terra: PSP_010852_1735 ESP_051743_1735 (Interval in Earth days: 3186) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.41 | 81.6 | 6.01 | -16.4 | 57.8 | 48.3 |
| Erosional Remnants on Ganges Mensa: ESP_011582_1730 ESP_011648_1730 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.16 | 311. | 6.37 | -16.2 | 57.0 | 58.6 |
| Very Fresh 1-Kilometer Crater: PSP_010571_2205 ESP_016083_2205 (Interval in Earth days: 429) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.22 | 187. | 0.52 | -26.3 | 53.7 | 46.1 |
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