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.
| Northern Mid-Latitude Crater: ESP_062806_2150 ESP_062740_2150 (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 | 34.80 | 100. | -3.6 | 15.57 | 45.8 | 43.6 |
| Terraced Fan in East Candor Chasma: ESP_062786_1730 ESP_062997_1730 (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 | -6.84 | 292. | -3.2 | -17.8 | 58.1 | 59.1 |
| Sinuous Inverted Channel in Large Basin in East Arabia Terra: ESP_062808_2085 ESP_062874_2085 (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 | 28.26 | 45.7 | 8.60 | -12.7 | 45.0 | 47.3 |
| Flow Deposits in Eastern Ladon Valles Basin: ESP_062745_1615 ESP_062956_1615 (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 | -18.2 | 332. | 8.06 | -7.02 | 64.1 | 64.6 |
| Dark Sediments in Medusae Fossae Formation: ESP_062791_1800 ESP_035679_1800 (Interval in Earth days: 2113) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.052 | 153. | 5.36 | 4.584 | 54.0 | 54.3 |
| 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 |
| Lyot Crater Peak Ring: ESP_062703_2295 ESP_062769_2295 (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 | 49.32 | 29.0 | 8.48 | -6.30 | 45.9 | 47.7 |
| 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 |
| 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 |
| 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 |
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