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.
| Hebes Chasma: ESP_037705_1790 ESP_046659_1790 (Interval in Earth days: 698) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.05 | 283. | -2.8 | 8.6 | 56.8 | 50.8 |
| Light-Toned Deposits in Noctis Labyrinthus: ESP_037732_1740 ESP_046752_1740 (Interval in Earth days: 703) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.06 | 267. | 2.13 | -10.1 | 57.0 | 52.5 |
| Crater Floor: ESP_037851_1780 ESP_038405_1780 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.92 | 257. | 12.7 | -0.09 | 55.8 | 56.6 |
| Well-Preserved Impact Crater Near Meroe Patera: ESP_037726_1870 ESP_046179_1870 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.943 | 70.0 | -6.2 | -20.9 | 56.9 | 51.3 |
| Oxia Palus: ESP_037729_1880 ESP_037874_1880 (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 | 7.808 | 348. | -13. | 8.553 | 57.6 | 56.4 |
| Arabia Terra: ESP_037741_2025 ESP_067953_2025 (Interval in Earth days: 2354) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.28 | 17.5 | 6.15 | -16.4 | 57.6 | 47.6 |
| Light-Toned Deposits Exposed along Floor of Terra Sabaea Crater: ESP_037673_1550 ESP_038240_1550 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -24.8 | 80.8 | -6.4 | 23.83 | 62.4 | 55.3 |
| Crater in Tempe Terra: ESP_037691_2170 ESP_045999_2170 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.64 | 299. | 13.0 | -7.66 | 60.2 | 51.0 |
| InSight Mission Candidate Landing Site: ESP_037829_1840 ESP_038383_1840 (Interval in Earth days: 43) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 3.983 | 137. | 10.4 | -4.64 | 55.9 | 58.2 |
| Channel Intersection with Aram Chaos: ESP_037782_1825 ESP_038402_1825 (Interval in Earth days: 48) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 2.655 | 340. | 5.31 | -25.6 | 56.2 | 59.7 |
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