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.
| Proposed Site for Future Exploration in Nili Fossae Carbonate Plains: ESP_032728_2020 ESP_032873_2020 (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 | 21.73 | 79.0 | 5.29 | 19.71 | 39.8 | 37.9 |
| Thermokarst: ESP_032872_1405 ESP_040837_1405 (Interval in Earth days: 621) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.2 | 116. | -3.2 | -16.8 | 52.1 | 41.5 |
| Gullies and Lobes in Crater in Terra Sirenum: ESP_032539_1330 ESP_058952_1330 (Interval in Earth days: 2059) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -46.5 | 208. | 2.89 | -17.3 | 51.2 | 50.7 |
| Gullies in Bogia Crater: ESP_032504_1355 ESP_033150_1355 (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 | -44.1 | 83.0 | 7.64 | 28.51 | 48.7 | 58.4 |
| Migrating and Static Sand Ripples on Mars: ESP_032616_1275 ESP_032748_1275 (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 | -52.2 | 267. | 3.02 | -26.0 | 56.8 | 60.7 |
| Lava against an Impact Crater in Elysium Planitia: ESP_018537_1860 ESP_019170_1860 (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 | 5.980 | 150. | 5.55 | -19.2 | 51.1 | 53.8 |
| Possible Cyclic Bedding within a Crater in Arabia Terra: ESP_018714_1890 ESP_019347_1890 (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 | 8.969 | 358. | 6.46 | -18.9 | 50.0 | 53.4 |
| Probable Impact Crater in South Polar Layered Deposits: ESP_032212_0905 ESP_041127_0905 (Interval in Earth days: 695) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -89.3 | 168. | 28.9 | 27.20 | 78.7 | 80.5 |
| Lava Flow in Syria Planum: ESP_032326_1605 ESP_032827_1605 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.1 | 259. | 7.00 | 25.67 | 33.4 | 37.6 |
| Exposure of South Polar Layered Deposits: ESP_032401_0920 ESP_032650_0920 (Interval in Earth days: 19) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -87.9 | 93.8 | 8.93 | 20.48 | 82.8 | 85.6 |
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