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.
| Crater in Arabia Terra: ESP_067808_2205 ESP_067465_2205 (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 | 40.14 | 7.67 | 11.8 | -4.93 | 56.5 | 61.7 |
| Cones in Chryse Planitia: ESP_068087_1990 ESP_067691_1990 (Interval in Earth days: 31) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 18.98 | 323. | -21. | 5.62 | 46.4 | 45.9 |
| Features in Echus Chasma: ESP_068049_1805 ESP_072665_1805 (Interval in Earth days: 360) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 0.707 | 279. | 4.52 | 27.80 | 41.1 | 54.4 |
| Troughs and Ridges in Chryse Planitia: ESP_067955_2110 ESP_072492_2110 (Interval in Earth days: 353) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.75 | 321. | -6.7 | 11.33 | 50.8 | 53.9 |
| Lobate Debris Apron on Floor of Barnard Crater: ESP_067833_1185 ESP_067688_1185 (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 | -61.0 | 60.2 | 11.4 | -14.6 | 64.7 | 63.7 |
| Ejecta on Icy Crater Fill: ESP_067922_2205 ESP_064268_2205 (Interval in Earth days: 284) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.10 | 139. | -6.1 | 21.82 | 56.4 | 62.6 |
| Fresh 1.5-Kilometer Crater: ESP_067862_2105 ESP_086825_2105 (Interval in Earth days: 1477) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 30.35 | 337. | 2.63 | 16.24 | 50.7 | 40.4 |
| Pitted Mounds in Aurorae Chaos: ESP_067955_1730 ESP_073626_1730 (Interval in Earth days: 442) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.78 | 324. | 4.46 | 25.36 | 40.8 | 54.4 |
| Mounds in Chryse Planitia: ESP_067915_2000 ESP_067506_2000 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.76 | 330. | 21.7 | 6.28 | 43.8 | 47.6 |
| Troughs and Ridges in Chryse Planitia: ESP_067823_2105 ESP_067480_2105 (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 | 30.33 | 319. | 13.9 | -5.70 | 50.2 | 54.9 |
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