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.
| Recent Crater in Southern Mid-Latitudes: ESP_066067_1350 ESP_066476_1350 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -44.6 | 8.27 | -1.5 | -22.4 | 44.2 | 43.5 |
| Gullies in Promethei Terra Crater: ESP_065866_1360 ESP_066011_1360 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.7 | 93.7 | -4.1 | 22.17 | 46.3 | 42.7 |
| Ares Vallis: ESP_065791_1920 ESP_066200_1920 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.67 | 333. | -3.6 | -25.0 | 60.4 | 58.6 |
| Raided Curvilinear Ridges: ESP_066022_1755 ESP_065956_1755 (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 | -4.63 | 151. | -7.5 | 6.58 | 50.4 | 50.1 |
| Outflow Channel from Morella Crater: ESP_065792_1700 ESP_057880_1700 (Interval in Earth days: 617) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.85 | 309. | -13. | 5.997 | 51.0 | 33.6 |
| Low Thermal Inertia Mound in Terra Sabaea Bedrock Plain: ESP_066039_1605 ESP_074968_1605 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.0 | 48.7 | -2.1 | 8.696 | 44.8 | 41.0 |
| Gullies: ESP_065810_1335 ESP_066839_1335 (Interval in Earth days: 80) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.3 | 182. | -5.6 | -23.1 | 47.5 | 44.7 |
| Athabasca Valles Distributary: ESP_066035_1875 ESP_057978_1875 (Interval in Earth days: 627) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.385 | 153. | 7.18 | -7.96 | 55.4 | 42.4 |
| Debris Flows on Eos Chasma Walls: ESP_065950_1665 ESP_065884_1665 (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 | -13.3 | 317. | -8.6 | 5.799 | 47.8 | 47.5 |
| Drainage Features South of Orson Welles Crater: ESP_066082_1780 ESP_074721_1780 (Interval in Earth days: 673) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.05 | 313. | -4.7 | -20.6 | 50.8 | 52.2 |
Page 213 of 878 (8,771 images) | |||||