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 Landing Site for SpaceX Starship East of Arcadia Planitia: ESP_060732_2195 ESP_060376_2195 (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 | 39.09 | 196. | 29.4 | 18.03 | 37.3 | 39.3 |
| Pitted Material on Floor of Ellsley Crater in Tempe Fossae: ESP_060716_2165 ESP_060782_2165 (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 | 36.27 | 276. | 8.42 | -7.32 | 38.7 | 40.0 |
| Small Scale Lava Flow Morphology in Daedalia Planum: ESP_060863_1540 ESP_060929_1540 (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 | -25.9 | 232. | 2.34 | -17.3 | 63.6 | 65.4 |
| Potential Lava Flow in Xanthe Terra: ESP_060807_1785 ESP_060873_1785 (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 | -1.40 | 318. | 1.40 | -19.1 | 47.4 | 49.5 |
| Candidate Landing Site for 2020 Mission in Jezero Crater: ESP_060829_1985 ESP_062161_1985 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.45 | 77.0 | -19. | -28.8 | 41.5 | 47.5 |
| Faulted and Embayed Low Shield East of Pavonis Mons: ESP_060783_1800 ESP_061139_1800 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.196 | 253. | -5.6 | 17.40 | 46.9 | 48.0 |
| Unusual Circular Depressions around Naar Crater: ESP_060741_2030 ESP_061730_2030 (Interval in Earth days: 77) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.97 | 317. | -7.8 | 18.30 | 39.5 | 40.7 |
| Two Small Cones in Hydraotes Chaos: ESP_060266_1795 ESP_060754_1795 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.34 | 326. | 6.09 | -16.5 | 41.3 | 47.7 |
| Fissure Adjacent to Olympica Fossae: ESP_060282_2055 ESP_060427_2055 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 25.36 | 246. | 1.79 | 18.58 | 37.4 | 36.2 |
| Light-Toned Deposits along Ius Chasma Wallrock: ESP_060479_1730 ESP_060835_1730 (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 | -7.15 | 273. | -9.0 | 12.07 | 48.0 | 50.2 |
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