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.
| Meridiani Planum Terrain Sample: ESP_026283_1810 ESP_026415_1810 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 1.156 | 354. | 26.9 | -16.8 | 49.2 | 52.9 |
| Exposure of Nili Fossae Megabreccias: ESP_026346_2000 ESP_026491_2000 (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 | 19.73 | 74.0 | 1.32 | 16.62 | 42.9 | 42.0 |
| Eastern Rim of Karzok Crater: ESP_026314_1985 ESP_026670_1985 (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 | 18.39 | 228. | -5.3 | 6.588 | 43.7 | 43.8 |
| Dune Changes in North Polar Crater: ESP_026404_2565 ESP_026457_2565 (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 | 76.14 | 270. | 13.7 | -2.98 | 53.3 | 54.3 |
| Olympica Fossae: ESP_026287_2050 ESP_025654_2050 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.58 | 245. | -11. | 3.311 | 42.4 | 39.5 |
| Craters and Mesas in Northeast Arabia Terra: ESP_026254_2085 ESP_026399_2085 (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 | 28.09 | 65.4 | -7.4 | 6.562 | 41.3 | 40.5 |
| Dune Changes in Vastitas Borealis Crater: ESP_026271_2515 ESP_026047_2515 (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 | 71.16 | 309. | 6.53 | -8.67 | 51.0 | 52.8 |
| Banded Terrain in Hellas Planitia: ESP_026360_1415 ESP_026426_1415 (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 | -38.0 | 57.4 | 19.2 | 1.121 | 77.1 | 78.3 |
| Sharp-Rimmed Crater on Northern Plains: ESP_026383_2465 ESP_026673_2465 (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 | 66.00 | 137. | -7.2 | 4.831 | 49.1 | 48.3 |
| Well-Exposed Bedrock Layers in Northern Hellas Planitia: ESP_026492_1540 ESP_036052_1540 (Interval in Earth days: 745) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -25.9 | 54.4 | -4.8 | 7.826 | 70.0 | 70.5 |
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