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.
Ejecta and Interior of Gamboa Crater: PSP_010896_2210 ESP_028025_2210 (Interval in Earth days: 1335) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.80 | 315. | -8.5 | 7.506 | 58.9 | 49.2 |
Outcrops of Light-Toned Materials Exposed in Highlands Crater Wall: PSP_010448_1530 ESP_016751_1530 (Interval in Earth days: 491) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.7 | 315. | -5.7 | 11.67 | 68.8 | 64.8 |
Knobs and Thermokarst: ESP_011365_1365 ESP_011642_1365 (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 | -43.3 | 120. | 5.79 | -16.4 | 67.6 | 65.5 |
Fresh Impact Crater on Northern Plains: PSP_010441_2385 PSP_010810_2385 (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 | 58.19 | 135. | -7.9 | 20.93 | 58.0 | 61.1 |
Possible Active Geyser Locale: ESP_011406_0945 ESP_011407_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 | -85.4 | 103. | 14.4 | -9.73 | 87.5 | 89.6 |
Fresh Unnamed Crater in Northern Hesperia Planum: ESP_011339_1665 ESP_011972_1665 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.1 | 106. | 5.47 | -13.2 | 58.4 | 56.8 |
Characterize Surface Hazards and Science of Possible MSL Rover Landing Site: PSP_010540_1535 PSP_010685_1535 (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 | -26.2 | 325. | -23. | -11.7 | 69.3 | 67.5 |
Large Clay and Chloride Exposure in Southeast Sirenum Fossae Region: PSP_010900_1405 ESP_016201_1405 (Interval in Earth days: 413) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 216. | -5.2 | -28.4 | 71.9 | 69.5 |
Light-Toned Layering along Wallrock in Southwest Melas Chasma: ESP_011504_1700 ESP_016106_1700 (Interval in Earth days: 359) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.99 | 284. | -28. | -15.4 | 60.3 | 48.7 |
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 |
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