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.
| 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 |
| Layered Terrain in Aeolis Planum: ESP_018181_1730 ESP_018893_1730 (Interval in Earth days: 55) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.83 | 152. | -5.0 | 11.41 | 58.6 | 56.8 |
| Cones at Edge of North Polar Layered Deposits: ESP_018334_2600 ESP_026641_2600 (Interval in Earth days: 647) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.05 | 275. | -5.1 | 10.19 | 58.7 | 56.0 |
| Kasei Valles North Wall Terraces: ESP_018149_2060 ESP_018439_2060 (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 | 25.94 | 302. | -8.0 | 18.69 | 44.6 | 43.2 |
| Rim and Ejecta of Very Fresh 7-Kilometer Diameter Impact Crater: ESP_018268_2335 ESP_033854_2335 (Interval in Earth days: 1215) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 53.34 | 289. | -4.9 | 20.21 | 46.1 | 47.4 |
| 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 |
| 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 |
| Cones at Edge of North Polar Layered Deposits: ESP_018241_2595 ESP_027063_2595 (Interval in Earth days: 688) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.12 | 293. | -0.4 | -20.8 | 57.4 | 58.6 |
| Well-Preserved 5-Kilometer Diameter Crater South of Isidis Planitia: ESP_018447_1750 ESP_018948_1750 (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 | -5.18 | 90.0 | -4.4 | 18.17 | 57.6 | 55.4 |
Page 681 of 900 (8,995 images) | |||||