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 Continuous Ejecta Boundary of Noord Crater in Noachis Terra: ESP_063997_1610 ESP_064063_1610 (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 | -18.9 | 348. | 2.28 | -20.1 | 60.7 | 62.1 |
| Dune Field: ESP_063747_2450 ESP_063523_2450 (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 | 64.50 | 315. | 23.6 | 6.414 | 64.0 | 61.8 |
| North Polar Residual Cap: ESP_063730_2680 ESP_063428_2680 (Interval in Earth days: 24) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.68 | 45.5 | -19. | -29.8 | 79.3 | 75.6 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_063453_1985 ESP_063519_1985 (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 | 18.07 | 77.1 | -3.2 | -24.5 | 51.6 | 54.0 |
| Medusae Fossae Formation above Athabasca Valles Lavas: ESP_063780_1840 ESP_063925_1840 (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 | 3.899 | 150. | -4.4 | 9.655 | 55.5 | 54.9 |
| Steep Slopes and Dunes in East Coprates Chasma: ESP_063524_1650 ESP_063458_1650 (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 | -14.6 | 302. | 0.84 | 24.26 | 60.7 | 59.1 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_063760_1990 ESP_063826_1990 (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 | 18.63 | 335. | -3.2 | -23.6 | 54.1 | 56.6 |
| Pit in Hephaestus Fossae: ESP_063504_1995 ESP_055262_1995 (Interval in Earth days: 642) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.50 | 124. | 1.15 | -17.0 | 51.6 | 54.3 |
| Possible Deltas in Crater in Amazonis Planitia: ESP_063462_1985 ESP_063752_1985 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.27 | 190. | 8.53 | 29.19 | 50.7 | 51.0 |
| Crater Floor Deposits with Possible Fan Delta and Shallow Valleys: ESP_063759_2175 ESP_046656_2175 (Interval in Earth days: 1333) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.11 | 1.65 | -17. | 0 | 57.7 | 59.7 |
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