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.
| Lava-Covered Crater in Kasei Valles: ESP_033709_2040 ESP_033999_2040 (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 | 23.79 | 296. | -8.4 | 21.43 | 39.6 | 37.6 |
| Becquerel Crater Dune Changes: ESP_033707_2015 ESP_034419_2015 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.23 | 351. | -10. | 10.77 | 39.6 | 40.3 |
| Valleys in Crater Northwest of Hellas Planitia: ESP_033956_1580 ESP_042277_1580 (Interval in Earth days: 648) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -21.7 | 38.1 | -0.9 | -11.6 | 56.9 | 51.2 |
| Kasei Valles Flow: ESP_033775_2075 ESP_034276_2070 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.93 | 293. | -2.8 | 24.56 | 39.6 | 37.9 |
| Well-Preserved Impact Crater in Tyrrhena Terra: ESP_033822_1685 ESP_034099_1685 (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 | -11.5 | 95.0 | -0.3 | -25.1 | 49.0 | 53.9 |
| Valley in Pit Crater: ESP_033825_1695 ESP_034181_1695 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.2 | 12.3 | 7.27 | 21.71 | 47.8 | 50.8 |
| Aprons with Raised Edges: ESP_033779_2310 ESP_034069_2310 (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 | 50.43 | 180. | -2.9 | 17.05 | 48.1 | 44.6 |
| Fissure Near Cerberus Fossae: ESP_033793_1875 ESP_034426_1875 (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 | 7.606 | 163. | 8.31 | -7.39 | 39.9 | 45.9 |
| Possible Future Landing Site Near Eastern Valley of Jezero Crater: ESP_033717_1990 ESP_033651_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 | 18.68 | 78.1 | -3.6 | 17.07 | 38.9 | 36.9 |
| Sinuous Ridges in Aeolis Region: ESP_033820_1735 ESP_034176_1735 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.31 | 149. | -0.9 | 14.15 | 46.2 | 49.0 |
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