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.
| Phyllosilicate-Rich Central Pit and Landslide in Tyrrhena Terra: ESP_066117_1745 ESP_066183_1745 (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 | -5.62 | 78.7 | -5.8 | -21.9 | 48.9 | 49.3 |
| Inverted Channel in Naktong Vallis: ESP_066488_1875 ESP_066554_1875 (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 | 7.476 | 30.6 | 7.93 | -6.23 | 50.8 | 51.0 |
| Possible Volcanic Caldera in Terra Sirenum: ESP_066442_1530 ESP_067062_1530 (Interval in Earth days: 48) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.8 | 211. | -1.8 | 8.657 | 39.7 | 37.4 |
| West Half of Well-Preserved Crater in Margaritifer Terra: ESP_066437_1675 ESP_075168_1675 (Interval in Earth days: 680) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.5 | 345. | -3.1 | 28.39 | 42.6 | 39.0 |
| Ridge in Eastern Argyre Planitia: ESP_066161_1310 ESP_066517_1310 (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 | -48.7 | 326. | -26. | 7.845 | 46.5 | 42.7 |
| Inverted Layered Crater Fill: ESP_066202_1320 ESP_067033_1320 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -47.7 | 283. | 3.21 | 21.71 | 43.7 | 43.7 |
| Gullies in Promethei Terra Crater: ESP_066143_1360 ESP_065721_1360 (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 | -43.7 | 93.6 | 2.40 | -26.4 | 43.1 | 49.9 |
| Sinuous Ridges and Possible Layers: ESP_066186_1545 ESP_065711_1545 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.2 | 0.17 | -28. | 6.876 | 44.2 | 46.7 |
| Outlet Channel from Crater: ESP_066226_1460 ESP_066160_1460 (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 | -33.6 | 347. | -8.5 | 6.106 | 41.8 | 41.3 |
| Knobby South Polar Layered Deposits Exposure: ESP_066234_1070 ESP_066498_1070 (Interval in Earth days: 20) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -73.0 | 139. | -4.5 | -22.4 | 56.1 | 58.0 |
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