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.
| Possible Olivine-Rich Crater in Terra Sirenum: ESP_022952_1305 ESP_050327_1305 (Interval in Earth days: 2133) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -49.3 | 223. | -5.1 | 22.16 | 42.8 | 54.0 |
| Arabia Terra Crater Floor Dune Changes: ESP_022775_1930 ESP_022498_1930 (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 | 12.90 | 9.07 | -25. | 2.217 | 47.8 | 49.6 |
| Pavonis Mons Reticulate Bedform Changes: ESP_022819_1815 ESP_023175_1815 (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 | 1.407 | 247. | -6.6 | 4.929 | 39.0 | 34.9 |
| Possible Kaolinite Deposit on Kashira Crater Floor: ESP_023053_1525 ESP_029910_1525 (Interval in Earth days: 535) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.2 | 341. | 0 | 15.68 | 32.7 | 48.7 |
| Proposed Site for Future Exploration North of Hellas Planitia: ESP_022958_1540 ESP_023446_1540 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.8 | 54.8 | 6.17 | -23.4 | 31.8 | 36.8 |
| Dune Changes: ESP_022889_1080 ESP_022731_1080 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -71.6 | 142. | 24.2 | 0.004 | 56.6 | 56.2 |
| The Crazy Floor of the Hellas Basin: ESP_023234_1460 ESP_024091_1460 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.5 | 81.5 | 0.57 | 28.11 | 36.3 | 46.4 |
| Starburst Spiders at a South Polar Cracked and Gullied Site: ESP_023117_0980 ESP_022998_0980 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -81.6 | 66.2 | -18. | -2.77 | 70.6 | 67.8 |
| Fan-Shaped Deposit in a Valles Marineris Trough: ESP_022949_1650 ESP_030518_1650 (Interval in Earth days: 590) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.9 | 299. | -1.6 | 21.10 | 32.0 | 42.9 |
| Coprates Chasma Dune Changes: ESP_022369_1685 ESP_023002_1685 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.4 | 293. | 4.01 | -17.8 | 37.5 | 33.6 |
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