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.
| Relatively Fresh 1-Kilometer Diameter Crater in South Polar Region : ESP_013699_1055 ESP_013923_1055 (Interval in Earth days: 18) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -74.1 | 130. | -4.9 | 10.22 | 57.2 | 58.2 |
| Central Uplift of Well-Exposed Taytay Crater : ESP_012794_1875 ESP_012939_1875 (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 | 7.398 | 340. | 8.24 | 23.49 | 56.4 | 54.2 |
| Pit Crater Chain Southwest of Arsia Mons: ESP_014077_1660 ESP_058186_1660 (Interval in Earth days: 3437) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 236. | -3.3 | 8.798 | 34.6 | 29.8 |
| Strike Slip Fault in Amazonis Planitia: ESP_012799_1990 ESP_013076_1990 (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 | 18.75 | 203. | 1.92 | -21.6 | 63.2 | 63.0 |
| 5 Kilometer Diameter Impact Crater Northwest of Mojave Crater: ESP_013968_1890 ESP_014390_1890 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.866 | 328. | 6.90 | -3.58 | 44.6 | 40.6 |
| South Polar Layered Deposits Exposed in Ultimum Chasma: ESP_013619_0990 ESP_013672_0990 (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 | -80.8 | 151. | 18.0 | 4.365 | 60.2 | 61.5 |
| Raga Crater: ESP_014011_1315 ESP_014288_1315 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -48.1 | 242. | 1.60 | -18.1 | 41.9 | 45.6 |
| Interesting Contrasts in Gully Morphology: ESP_014104_1360 ESP_021686_1360 (Interval in Earth days: 591) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.8 | 222. | 3.50 | 25.74 | 40.1 | 42.0 |
| Stratigraphy of Rocks in Claritas Fossae Region: ESP_012995_1530 ESP_030902_1530 (Interval in Earth days: 1395) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -26.9 | 258. | -7.1 | 4.769 | 43.5 | 37.3 |
| Crossing Ridges in Dorsa Argentea: ESP_012729_1020 ESP_013032_1020 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -77.8 | 337. | -6.9 | 14.65 | 62.3 | 58.2 |
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