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.
| Buried Crater on Ice-Rich Plateau on Malea Patera: ESP_083065_1170 ESP_083289_1170 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -62.9 | 53.3 | -2.6 | 23.60 | 57.6 | 52.6 |
| Terrain Sample in Aeolis Planum: ESP_082969_1810 ESP_083892_1810 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.792 | 143. | 5.12 | -5.74 | 56.4 | 49.0 |
| Crater: ESP_083271_1585 ESP_083772_1585 (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 | -21.2 | 181. | 0 | 13.72 | 47.8 | 40.5 |
| Sinuous Ridge between Craters: ESP_083008_1690 ESP_083641_1690 (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 | -11.0 | 160. | 3.77 | -18.6 | 52.5 | 47.5 |
| Channel in Valley near Tyrrhena Patera: ESP_083076_1590 ESP_083142_1590 (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 | -20.6 | 104. | 3.93 | -19.6 | 50.0 | 51.0 |
| Sedimentary Fans in Crater: ESP_082930_1470 ESP_083141_1470 (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 | -32.7 | 132. | 8.74 | -2.72 | 51.1 | 49.0 |
| Athabasca Valles: ESP_083074_1895 ESP_083140_1895 (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 | 9.230 | 156. | -4.3 | -26.0 | 60.3 | 61.7 |
| Channels and Possible Deltas Southwest of Gale Crater: ESP_083009_1720 ESP_083497_1720 (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 | -7.81 | 132. | 0 | -28.2 | 53.7 | 51.2 |
| Pitted Material: ESP_083282_1425 ESP_083928_1425 (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 | -37.2 | 242. | 4.8 | 21.65 | 46.8 | 37.9 |
| Planned ExoMars Landing Site in Oxia Planum: ESP_083041_1980 ESP_082975_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 | 17.80 | 335. | 2.09 | 23.42 | 64.3 | 62.7 |
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