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.
| Fresh and Well-Preserved 20-Kilometer Diameter Impact Crater in Arabia Terr: ESP_018252_1965 ESP_018753_1965 (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 | 16.47 | 11.5 | -8.4 | 14.84 | 47.5 | 46.9 |
| Exposure of Putative Deformation in North Polar Layers: ESP_018361_2655 ESP_018810_2655 (Interval in Earth days: 35) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.20 | 242. | -4.5 | -18.9 | 62.0 | 66.4 |
| Pitted Terrain North of Hrad Vallis: ESP_018168_2160 ESP_019012_2160 (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 | 35.59 | 141. | -3.2 | -24.7 | 43.1 | 50.1 |
| Central Uplift of Impact Crater: ESP_018277_1620 ESP_026202_1620 (Interval in Earth days: 618) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.5 | 52.1 | 3.42 | -23.2 | 65.0 | 64.1 |
| Light-Toned Outcrops in Noctis Region: ESP_018124_1720 ESP_018757_1720 (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 | -8.00 | 268. | 0.79 | -20.5 | 59.0 | 59.9 |
| Noctis Labyrinthus Terrain: ESP_018441_1735 ESP_045579_1735 (Interval in Earth days: 2115) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.28 | 253. | -2.1 | -25.1 | 58.1 | 55.0 |
| Longitudinally Aligned Cones: ESP_018457_2065 ESP_018747_2065 (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 | 26.25 | 173. | -8.5 | 18.07 | 45.6 | 44.5 |
| Fresh 2-Kilometer Diameter Impact Crater: ESP_018219_2155 ESP_078576_2155 (Interval in Earth days: 4702) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.25 | 189. | -0.7 | 11.46 | 43.1 | 41.8 |
| Mass Wasting on Steep North-Polar Boundary Scarp: ESP_018115_2640 ESP_018932_2640 (Interval in Earth days: 63) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.82 | 121. | -0.2 | 13.54 | 59.8 | 65.3 |
| Cerberus Fossae Fissure and Lava Flows: ESP_018141_1965 ESP_018774_1965 (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 | 16.06 | 160. | 6.15 | -13.7 | 46.3 | 49.4 |
Page 666 of 885 (8,850 images) | |||||