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.
| Landforms Near Gale Crater Central Peak : ESP_053310_1745 ESP_053033_1745 (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 | -5.30 | 138. | -13. | 21.28 | 56.0 | 53.2 |
| Well-Preserved Impact Crater on Northern Plains : ESP_053514_2170 ESP_060833_2170 (Interval in Earth days: 570) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.82 | 322. | -4.2 | 12.83 | 41.3 | 38.4 |
| Exposure of North Polar Layered Deposits : ESP_053454_2670 ESP_053429_2670 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 87.07 | 92.9 | 0.40 | -13.6 | 62.8 | 62.7 |
| Floor of Melas Chasma : ESP_053423_1690 ESP_060452_1690 (Interval in Earth days: 547) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.7 | 290. | 19.4 | -1.79 | 57.3 | 49.2 |
| Small Well-Preserved and Potentially Gullied Crater in Idaeus Fossae : ESP_053488_2195 ESP_053923_2195 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.97 | 311. | -2.4 | 26.94 | 41.2 | 40.8 |
| Chaos Terrain Near Eos Chasma : ESP_053488_1635 ESP_061150_1635 (Interval in Earth days: 597) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -16.3 | 319. | -8.6 | -24.8 | 62.8 | 61.2 |
| Pitted Cones in Chryse Planitia : ESP_053527_2160 ESP_053817_2160 (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 | 35.45 | 326. | 1.07 | 22.02 | 40.9 | 40.4 |
| Flattop Dunes Near Gypsum Source : ESP_053358_2600 ESP_053477_2600 (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 | 79.98 | 240. | 6.81 | -8.75 | 56.5 | 57.8 |
| Terrain along Hebes Mensa: ESP_053265_1785 ESP_053054_1785 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.32 | 283. | 14.8 | 24.92 | 51.6 | 50.5 |
| Dunes Dubbed Chusuk : ESP_053590_2570 ESP_053643_2570 (Interval in Earth days: 4) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 76.84 | 30.2 | 8.90 | -7.27 | 55.3 | 56.7 |
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