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.
| Irregular Circular Depressions near Makhambet Crater: ESP_062798_2105 ESP_062864_2105 (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 | 30.04 | 320. | -6.4 | -25.4 | 46.1 | 48.4 |
| Chasma Boreale Megadunes: ESP_062652_2630 ESP_062547_2630 (Interval in Earth days: 8) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.75 | 315. | 7.01 | -8.83 | 61.2 | 61.3 |
| Translucent Ice on Dunes: ESP_062996_2550 ESP_072057_2550 (Interval in Earth days: 706) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.98 | 300. | 2.86 | 20.32 | 60.1 | 62.4 |
| Ridges in Arcadia Planitia: ESP_062856_2265 ESP_062922_2265 (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 | 46.36 | 172. | 8.39 | -7.31 | 46.6 | 48.6 |
| 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_062741_1990 ESP_063387_1990 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.68 | 77.2 | 0.54 | 17.50 | 47.1 | 49.4 |
| 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 |
| 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 |
| 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 |
| Dunes Dubbed Hazar: ESP_062627_2555 ESP_054029_2555 (Interval in Earth days: 670) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 75.24 | 293. | 7.72 | -8.08 | 56.3 | 58.9 |
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