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.
| Bench in Samara Valles: ESP_090425_1545 ESP_090715_1545 (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 | -25.0 | 340. | 3.09 | 12.71 | 63.4 | 60.4 |
| An Inverted Channel in Flammarion Crater: ESP_089631_2065 ESP_090330_2065 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.02 | 48.9 | 5.65 | -12.0 | 49.6 | 57.2 |
| Deep in Valles Marineris: ESP_089134_1655 ESP_088633_1655 (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 | -14.3 | 303. | -5.3 | -18.1 | 64.4 | 65.7 |
| Possible Skylight Showing Thermal Anomaly in Young Lava Flows: ESP_089930_1890 ESP_090286_1890 (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 | 8.718 | 169. | -5.8 | 16.74 | 54.6 | 54.1 |
| Fracture near Double Crater: ESP_090204_1700 ESP_090349_1700 (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 | -9.67 | 251. | 6.04 | 28.44 | 58.8 | 56.7 |
| Knobs in Arcadia Planitia: ESP_090206_2220 ESP_090483_2220 (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 | 41.62 | 189. | 5.61 | -6.01 | 57.5 | 62.4 |
| Landing Site Characterization for Possible Future Rotorcraft : ESP_090127_2185 ESP_089204_2185 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.18 | 186. | 4.89 | -13.2 | 55.7 | 48.1 |
| Lava Falls in Kasei Valles: ESP_089952_2025 ESP_090097_2025 (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 | 22.09 | 286. | 7.26 | 24.46 | 52.0 | 51.6 |
| Light-Toned Exposures on Floor of Coprates Chasma: ESP_090202_1645 ESP_090479_1645 (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 | -15.3 | 306. | 4.32 | -12.0 | 60.9 | 61.0 |
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_090006_2240 ESP_090362_2240 (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 | 43.48 | 249. | 2.39 | 19.01 | 55.5 | 59.1 |
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