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.
| Lethe Vallis Features: ESP_083852_1845 ESP_084076_1845 (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 | 4.307 | 155. | -8.8 | 26.04 | 51.6 | 46.6 |
| Crater with Hydration Signatures in West Hellas Planitia: ESP_083988_1400 ESP_084568_1400 (Interval in Earth days: 45) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.7 | 47.2 | -0.7 | 13.85 | 39.6 | 37.9 |
| Promethei Lingula Surface Roughness: ESP_083960_0975 ESP_066460_0975 (Interval in Earth days: 1363) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -82.5 | 108. | 8.61 | -6.04 | 61.5 | 63.4 |
| Sinuous Ridges and Lobate Debris Aprons on Edge of Argyre Planitia: ESP_083886_1235 ESP_084097_1235 (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 | -56.0 | 314. | 5.91 | -9.43 | 45.4 | 46.0 |
| Contacts between Likely Sulfates and Chaos Blocks in Eastern Iani Chaos: ESP_083766_1770 ESP_084056_1770 (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 | -3.09 | 344. | -8.5 | 2.235 | 48.7 | 44.5 |
| Athabasca Valles Distributary: ESP_083997_1885 ESP_084221_1885 (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 | 8.310 | 155. | -7.8 | 20.33 | 52.2 | 47.7 |
| Unit Margin and Pit: ESP_083989_1115 ESP_084121_1115 (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 | -68.3 | 25.5 | 4.01 | -20.4 | 52.2 | 54.0 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_083463_1980 ESP_083397_1980 (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 | 17.95 | 335. | -3.6 | 14.43 | 63.2 | 62.4 |
| Pyroxene-Rich Materials Surrounding Crater in Northeast Hellas Planitia: ESP_083367_1465 ESP_083789_1465 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.3 | 82.0 | 4.33 | -20.4 | 45.4 | 42.1 |
| Scarp in Hellas Planitia with Linear Gullies: ESP_083473_1315 ESP_083684_1315 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.0 | 70.6 | 4.47 | -8.56 | 46.2 | 44.9 |
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