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.
| Iani Chaos: ESP_063206_1780 ESP_063852_1780 (Interval in Earth days: 50) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.13 | 343. | 3.24 | 27.44 | 55.5 | 54.1 |
| Chasma Boreale Head Scarp Dunes: ESP_063323_2650 ESP_063441_2650 (Interval in Earth days: 9) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.69 | 0.77 | -8.0 | 6.363 | 70.6 | 71.6 |
| Small Ice-Filled North Polar Layered Deposits Crater: ESP_063253_2655 ESP_071615_2655 (Interval in Earth days: 651) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.65 | 93.4 | 0.84 | 10.75 | 69.9 | 64.7 |
| Layering in Arabia Terra: ESP_063337_1820 ESP_063403_1820 (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 | 1.753 | 6.72 | -6.4 | -28.7 | 55.0 | 57.0 |
| Pitted Mounds in Chryse Planitia: ESP_063325_2215 ESP_055307_2215 (Interval in Earth days: 624) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 41.11 | 331. | -26. | -6.76 | 53.9 | 60.3 |
| Cratered Cone North of Noctis Fossae: ESP_063209_1800 ESP_063420_1800 (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 | -0.10 | 261. | 0.69 | -12.9 | 54.8 | 56.2 |
| Possible Impact Melt Deposits in a Multiple Impact Structure: ESP_062296_1840 ESP_062586_1840 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.036 | 349. | 5.58 | 22.88 | 51.2 | 50.4 |
| Dynamic Activity in a Crater North of Antoniadi Crater : ESP_023261_2065 ESP_023327_2065 (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 | 26.12 | 57.0 | -1.8 | -18.8 | 49.3 | 49.4 |
| Pollywog Craters on Mars: ESP_061768_2200 ESP_062045_2200 (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 | 39.79 | 0.03 | -0.9 | -11.2 | 40.7 | 42.4 |
| Layered Bedrock in the Central Uplift of Betio Crater: ESP_016805_1565 ESP_017583_1565 (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 | -23.1 | 281. | 3.96 | -9.12 | 63.3 | 68.9 |
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