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.
| Layers in Crater: ESP_062819_2570 ESP_062661_2570 (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 | 76.98 | 88.7 | 7.47 | -6.37 | 59.0 | 58.5 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_062662_1990 ESP_062952_1990 (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 | 18.61 | 77.2 | -29. | -12.5 | 49.4 | 49.2 |
| Layered Material and Wall Spur in East Candor Chasma: ESP_062852_1725 ESP_069408_1725 (Interval in Earth days: 511) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.27 | 289. | 4.20 | -7.91 | 57.8 | 58.4 |
| High-Latitude Crater with Patterned Ground: ESP_062992_2475 ESP_063216_2475 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.07 | 55.0 | -2.5 | 13.10 | 56.3 | 57.9 |
| High-Latitude Lobate Slope Features: ESP_062735_2495 ESP_062959_2495 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 69.49 | 232. | -6.9 | 7.134 | 55.1 | 56.4 |
| Layering in Medusae Fossae Formation: ESP_062632_1715 ESP_062843_1715 (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 | -8.41 | 177. | -7.3 | -22.0 | 59.3 | 60.3 |
| Dunes Dubbed Hazar South: ESP_062970_2550 ESP_062838_2550 (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 | 74.99 | 293. | -6.2 | 5.004 | 60.4 | 58.2 |
| An Impact North of Valles Marineris: ESP_011425_1775 ESP_012282_1775 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.35 | 278. | -7.2 | 29.98 | 58.0 | 53.4 |
| The Life of a Glacier on Mars: PSP_008809_2215 PSP_009455_2215 (Interval in Earth days: 51) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.27 | 54.7 | -6.7 | 10.01 | 42.9 | 43.4 |
| Central Peak of a Large Crater: ESP_014361_1585 ESP_021587_1585 (Interval in Earth days: 563) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.5 | 44.7 | -14. | 6.137 | 35.0 | 43.9 |
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