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.
| Scalloped Terrain: PSP_001331_2260 PSP_002162_2260 (Interval in Earth days: 64) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.62 | 93.6 | 0 | 19.66 | 49.3 | 58.2 |
| Athabasca Valles Distributary Channel: PSP_001540_1890 PSP_002371_1890 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.783 | 155. | 16.5 | -3.96 | 50.4 | 55.2 |
| Layering in Danielson Crater : PSP_002944_1880 ESP_019835_1880 (Interval in Earth days: 1317) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.951 | 352. | -11. | 10.60 | 58.1 | 52.8 |
| North Polar Layered Deposits Exposed Wall: PSP_001488_2665 ESP_019158_2665 (Interval in Earth days: 1377) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 86.50 | 80.0 | 0.47 | -8.93 | 70.0 | 70.7 |
| Layers on Floor of West Candor Chasma: PSP_002195_1745 PSP_002406_1745 (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 | -5.19 | 282. | -5.3 | -11.5 | 56.6 | 56.9 |
| Fan Near Aeolis Mensae: PSP_002002_1735 PSP_002279_1735 (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 | -6.24 | 151. | 1.29 | -26.9 | 56.5 | 58.6 |
| Dark Materials on Block in Olympus Mons Aureole : PSP_002461_1975 ESP_011282_1975 (Interval in Earth days: 687) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.06 | 217. | -4.5 | 16.43 | 56.5 | 56.4 |
| Gullies in Dao Valles: PSP_001635_1445 PSP_001978_1445 (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 | -35.3 | 91.1 | 4.16 | -5.48 | 72.2 | 69.9 |
| Irregular Structures in Huo Hsing Vallis: PSP_002150_2110 PSP_002282_2110 (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 | 30.77 | 65.4 | 8.03 | -27.0 | 54.7 | 59.4 |
| Layering in Crater: PSP_002007_1800 PSP_002429_1800 (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 | -0.23 | 14.3 | 0 | -13.1 | 55.0 | 56.5 |
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