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.
| Basin in Northeast Hellas Region: ESP_026412_1525 ESP_026557_1525 (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 | -27.2 | 78.2 | 0 | 15.95 | 70.4 | 69.9 |
| 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 |
| Fresh Crater: ESP_026314_2390 ESP_025668_2390 (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 | 58.66 | 217. | 21.6 | 2.478 | 43.4 | 46.9 |
| 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 |
| Eastern Rim and Ejecta of Crater in Margaritifer Terra: ESP_026257_1605 ESP_026402_1605 (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 | -19.2 | 348. | -0.9 | 15.10 | 64.1 | 63.8 |
| Central Peak of Oudeman Crater: ESP_026550_1700 ESP_027117_1700 (Interval in Earth days: 44) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.72 | 268. | 4.52 | 16.91 | 58.4 | 58.1 |
| Proximal Region of Athabasca Valles: ESP_026554_1900 ESP_019829_1900 (Interval in Earth days: 524) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 9.961 | 157. | -5.2 | 1.324 | 47.9 | 53.4 |
| 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 |
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