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.
| Translucent Ice on Dunes: ESP_062996_2550 ESP_072057_2550 (Interval in Earth days: 706) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 74.98 | 300. | 2.86 | 20.32 | 60.1 | 62.4 |
| Ridges in Arcadia Planitia: ESP_062856_2265 ESP_062922_2265 (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 | 46.36 | 172. | 8.39 | -7.31 | 46.6 | 48.6 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_062662_1990 ESP_062952_1990 (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 | 18.61 | 77.2 | -29. | -12.5 | 49.4 | 49.2 |
| Dark Sediments in Medusae Fossae Formation: ESP_062791_1800 ESP_035679_1800 (Interval in Earth days: 2113) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.052 | 153. | 5.36 | 4.584 | 54.0 | 54.3 |
| High-Latitude Crater with Patterned Ground: ESP_062992_2475 ESP_063216_2475 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 67.07 | 55.0 | -2.5 | 13.10 | 56.3 | 57.9 |
| High-Latitude Lobate Slope Features: ESP_062735_2495 ESP_062959_2495 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 69.49 | 232. | -6.9 | 7.134 | 55.1 | 56.4 |
| Dunes Dubbed Hazar: ESP_062627_2555 ESP_054029_2555 (Interval in Earth days: 670) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 75.24 | 293. | 7.72 | -8.08 | 56.3 | 58.9 |
| Layering in Medusae Fossae Formation: ESP_062632_1715 ESP_062843_1715 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.41 | 177. | -7.3 | -22.0 | 59.3 | 60.3 |
| Fans or Lobes at Valley Terminus at Intersection of Crater Wall and Floor: ESP_062979_2015 ESP_063757_2015 (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 | 21.27 | 58.5 | -0.5 | -22.7 | 47.8 | 55.9 |
| Dunes Dubbed Hazar South: ESP_062970_2550 ESP_062838_2550 (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 | 74.99 | 293. | -6.2 | 5.004 | 60.4 | 58.2 |
Page 244 of 891 (8,901 images) | |||||