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.
| Well-Preserved Impact Crater: ESP_016884_2200 ESP_018229_2200 (Interval in Earth days: 104) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.69 | 276. | 1.9 | -10.3 | 41.3 | 44.0 |
| Small Rampart Crater Near the Central Peak of Lyot Crater: ESP_016326_2305 ESP_060026_2305 (Interval in Earth days: 3405) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 50.39 | 29.2 | -3.9 | 16.71 | 47.2 | 47.4 |
| Quasi-Periodic Layering in a Large Crater: ESP_016776_1810 ESP_016921_1810 (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 | 1.019 | 351. | -7.5 | 9.544 | 49.0 | 48.8 |
| Fractured and Deformed Crater Fill: ESP_016815_2145 ESP_017883_2145 (Interval in Earth days: 83) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.23 | 1.63 | -1.5 | 10.3 | 41.0 | 41.2 |
| Discontinuous Small Channel South of Dao Vallis: ESP_016311_1420 ESP_016588_1420 (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 | -37.6 | 89.5 | 5.56 | -17.0 | 67.7 | 72.4 |
| Submerged Rim of Crater and Floor Deposits from Uzboi Vallis: ESP_016487_1495 ESP_017120_1495 (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 | -30.0 | 323. | 11.7 | -6.42 | 64.1 | 71.3 |
| Lobate Tongue Terminus in CTX Image: ESP_016418_2255 ESP_017130_2255 (Interval in Earth days: 56) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 45.06 | 38.1 | -2.1 | 10.57 | 44.3 | 41.3 |
| Crosscutting Ridges beyond Margins of Mantle Material: ESP_016504_1410 ESP_019273_1410 (Interval in Earth days: 216) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.9 | 221. | -5.1 | 11.30 | 71.6 | 73.5 |
| Deposit Associated with Channels along Floor of Ganges Chasma: ESP_016817_1710 ESP_017239_1710 (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 | -8.69 | 311. | 5.05 | -13.5 | 53.8 | 57.9 |
| Crater with Perched Valleys in Claritas Fossae Region: ESP_016806_1405 ESP_016872_1405 (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 | -39.2 | 256. | 2.61 | -15.6 | 75.0 | 76.6 |
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