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.
| Layers Exposed on Arcuate Section of the North Polar Trough: ESP_037249_2665 ESP_037261_2665 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.32 | 94.6 | -8.4 | 6.669 | 77.4 | 77.3 |
| Valley System in Tempe Terra: ESP_037401_2235 ESP_037757_2235 (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 | 43.52 | 296. | -1.3 | 12.32 | 59.4 | 63.6 |
| Polar Crater Dune Changes: ESP_037330_2590 ESP_037422_2590 (Interval in Earth days: 7) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 79.09 | 60.9 | -1.3 | 14.61 | 74.0 | 74.6 |
| Layered Rocks of Ophir Mensa: ESP_037217_1760 ESP_036795_1760 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.95 | 286. | -3.9 | 17.29 | 57.2 | 55.7 |
| Candor Chasma: ESP_037586_1725 ESP_037731_1725 (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 | -7.41 | 293. | -8.5 | 13.50 | 58.2 | 56.3 |
| Crater on North Polar Layered Deposits: ESP_037296_2640 ESP_037322_2640 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.08 | 258. | -3.2 | 6.543 | 76.5 | 76.4 |
| Mound Surrounded by Lava Close to Noctis Fossae: ESP_037508_1800 ESP_064066_1800 (Interval in Earth days: 2069) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.04 | 261. | 3.98 | 19.18 | 55.9 | 55.0 |
| Landforms in Northern Lycus Sulci: ESP_037562_2125 ESP_037839_2125 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 32.13 | 223. | -1.0 | -16.0 | 58.3 | 63.1 |
| Possible Exposure of North Polar Layered Deposits: ESP_037227_2675 ESP_037305_2675 (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 | 87.48 | 319. | -8.6 | -2.75 | 77.9 | 79.3 |
| Intersection of Valley with Layered Plains: ESP_037529_2085 ESP_037463_2085 (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 | 28.23 | 45.4 | -9.2 | 8.55 | 57.8 | 55.6 |
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