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.
| Eastern Exposure of Hargraves Crater Ejecta: ESP_061040_2010 ESP_069442_2010 (Interval in Earth days: 655) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.61 | 76.7 | -16. | 7.667 | 41.8 | 47.9 |
| Glacial Features within Crater in Arabia Terra: ESP_061187_2155 ESP_087786_2155 (Interval in Earth days: 2072) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.14 | 19.9 | 4.85 | 25.65 | 39.1 | 40.0 |
| Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_061185_1985 ESP_060908_1985 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.43 | 77.0 | 2.38 | 19.53 | 41.4 | 38.7 |
| Crater with Exit Breach: ESP_061037_1375 ESP_061103_1375 (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 | -42.3 | 164. | 4.61 | -11.8 | 77.3 | 78.8 |
| Candidate Landing Site for SpaceX Starship Near Arcadia Planitia: ESP_061128_2190 ESP_061194_2190 (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 | 38.63 | 190. | 2.81 | -11.6 | 39.5 | 40.8 |
| Variety of Butte and Mesa-Forming Materials in Xanthe Terra: ESP_060926_1870 ESP_061704_1870 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 6.707 | 308. | -0.5 | 26.60 | 44.6 | 46.6 |
| Aeolian Units in South Melas Chasma: ESP_060729_1670 ESP_060795_1670 (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 | -13.0 | 289. | -0.6 | -20.8 | 53.6 | 55.6 |
| Complex Inverted Channels in Aeolis Dorsa: ESP_060734_1760 ESP_053639_1760 (Interval in Earth days: 552) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.00 | 153. | -26. | 5.933 | 50.2 | 53.9 |
| Pedestal Crater Near Phoenix Landing Site: ESP_060757_2485 ESP_060770_2485 (Interval in Earth days: 1) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.12 | 231. | -0.8 | 18.66 | 53.4 | 52.1 |
| Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_060763_1985 ESP_060697_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 | 18.46 | 77.1 | -1.0 | 17.86 | 39.7 | 37.8 |
Page 278 of 913 (9,124 images) | |||||