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.
| Central Peak of Trinidad Crater: PSP_009427_1565 ESP_027123_1565 (Interval in Earth days: 1378) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -23.4 | 109. | -2.9 | -19.4 | 70.1 | 69.3 |
| Seasonal Monitoring of Polar Crater with Summer Ice: PSP_009364_2505 ESP_018766_2505 (Interval in Earth days: 732) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 70.05 | 13.8 | -2.3 | -22.2 | 52.5 | 58.1 |
| Mounds in Ulysses Fossae: PSP_009409_1860 PSP_009554_1860 (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 | 5.804 | 237. | -7.2 | 8.646 | 53.1 | 52.1 |
| Potential Paleolake in Crater in Ophir Planum: PSP_010290_1700 PSP_010435_1700 (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 | -10.0 | 306. | 0.86 | 17.82 | 60.3 | 58.8 |
| Central Uplift of Hargraves Crater in the Nili Fossae Region: PSP_009639_2010 PSP_010272_2010 (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 | 20.73 | 75.8 | -5.4 | -21.0 | 47.8 | 52.1 |
| Impact Crater on Lava Flow Front in Amazonis Planitia: PSP_010109_1975 ESP_053848_1975 (Interval in Earth days: 3408) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.14 | 204. | -6.4 | 7.576 | 50.7 | 44.4 |
| Hydrated Light-Toned Layers on Crater Floor: PSP_010274_2140 PSP_010696_2140 (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 | 33.63 | 17.0 | 5.05 | -8.32 | 49.3 | 54.8 |
| Cones at Edge of North Polar Layered Deposits: PSP_009947_2590 PSP_009710_2590 (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 | 78.66 | 285. | 8.81 | -10.7 | 60.4 | 59.6 |
| Fresh 5-Kilometer Diameter Crater: PSP_009532_1640 PSP_010033_1640 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 121. | -7.7 | 17.88 | 65.2 | 62.7 |
| Tooting Crater Southern Ejecta Layer: PSP_009766_2030 PSP_009832_2030 (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 | 22.53 | 207. | 2.91 | -16.9 | 47.2 | 49.2 |
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