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.
| Candidate ExoMars Landing Site in Oxia Planum: ESP_072307_1985 ESP_072241_1985 (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 | 18.32 | 335. | -8.7 | 14.63 | 53.7 | 51.3 |
| Modification of Ringed Crater: ESP_072007_2485 ESP_072139_2485 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.45 | 234. | 8.48 | -8.32 | 59.3 | 62.3 |
| Small North Polar Layered Deposits Ice-Filled Crater: ESP_072184_2635 ESP_072224_2635 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.20 | 62.4 | 4.18 | -9.94 | 69.8 | 71.1 |
| Translucent Ice on Dunes South Site: ESP_072321_2550 ESP_072268_2550 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.99 | 299. | -1.4 | 17.00 | 67.7 | 65.6 |
| Dark Dune Field Topography in Bunge Crater: ESP_072374_1460 ESP_072440_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 | -33.4 | 311. | 11.1 | -11.4 | 70.3 | 71.2 |
| Rough Polar Terrain: ESP_072267_2575 ESP_072214_2575 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 77.12 | 332. | -1.2 | 14.67 | 68.0 | 66.1 |
| Channel in Cydonia Mensae: ESP_072201_2140 ESP_072412_2140 (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 | 33.59 | 347. | 2.53 | -10.0 | 51.9 | 55.3 |
| Mawrth Vallis Stratigraphy: ESP_072109_2015 ESP_072043_2015 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.23 | 341. | -4.2 | 18.87 | 51.8 | 49.3 |
| Crater in Arabia Terra: ESP_072398_2220 ESP_072464_2220 (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 | 41.47 | 6.12 | 8.82 | -8.40 | 55.0 | 57.3 |
| North Polar Residual Cap Topography: ESP_072114_2685 ESP_071770_2685 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.27 | 218. | -29. | -22.6 | 74.2 | 69.2 |
Page 159 of 878 (8,771 images) | |||||