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.
| Marte Vallis Channel between Crater Ejecta: ESP_033423_1970 ESP_033713_1970 (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 | 16.63 | 184. | -1.8 | 25.48 | 37.7 | 36.4 |
| Flow on Floor of Isil Crater: ESP_033585_1525 ESP_033730_1525 (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 | -27.3 | 87.8 | -5.6 | 9.704 | 55.7 | 56.9 |
| 12-Kilometer Diameter Crater with Multiple Pronounced Internal Morphologies: ESP_033317_1945 ESP_033462_1945 (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 | 14.33 | 199. | -1.3 | 12.06 | 37.2 | 36.6 |
| Monitoring Active Dunes in Arabia Terra: ESP_033456_1830 ESP_033601_1830 (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 | 3.139 | 4.55 | 11.1 | 24.90 | 38.0 | 38.1 |
| Pedestal Crater Modification: ESP_033663_2395 ESP_033953_2395 (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 | 59.21 | 104. | 6.93 | 21.26 | 53.6 | 49.9 |
| Pedestal Crater and Mantle: ESP_033612_2300 ESP_033744_2300 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.83 | 59.1 | 3.92 | -21.3 | 48.5 | 49.4 |
| Layered Materials on Northeast Hellas Planitia Rim: ESP_033348_1525 ESP_033282_1525 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.2 | 78.2 | -4.0 | 18.08 | 52.0 | 49.5 |
| Exposures of Light-Toned Layered Material along Ladon Valles Floor: ESP_033431_1585 ESP_033365_1585 (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 | -21.2 | 331. | 0.00 | 22.10 | 49.2 | 46.7 |
| Light-Toned Layered Deposits in Uplands West of Ladon Valles Basin: ESP_033352_1605 ESP_033774_1605 (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 | -19.4 | 327. | 4.51 | -10.4 | 46.7 | 53.6 |
| Ice-Rich Lobate Debris Apron: ESP_033363_2225 ESP_033653_2225 (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 | 42.08 | 18.5 | 7 | 25.58 | 46.0 | 42.5 |
Page 495 of 885 (8,850 images) | |||||