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.
| Reticulate Bedform Change Detection : ESP_049812_1735 ESP_050234_1735 (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 | -6.31 | 239. | 23.1 | 2.112 | 29.0 | 31.6 |
| Escarpment in North Tempe Terra : ESP_050074_2300 ESP_050285_2300 (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 | 49.44 | 279. | 4.48 | -4.93 | 61.4 | 58.8 |
| Candidate Landing Site for 2020 Mission in Northeast Syrtis Major Region : ESP_049752_1980 ESP_050042_1980 (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 | 17.85 | 77.0 | -16. | 18.40 | 43.0 | 37.9 |
| Pits in Valley on Rim of Moreux Crater : ESP_049819_2210 ESP_050096_2210 (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 | 40.81 | 44.0 | -4.0 | -23.6 | 58.5 | 55.8 |
| Lava Flows on Arsia Mons: ESP_049786_1615 ESP_049931_1615 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -18.2 | 232. | -5.0 | 19.84 | 31.2 | 30.3 |
| Mesa Island in East Acidalia Planitia : ESP_049834_2250 ESP_049966_2250 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.69 | 352. | 5.24 | -20.0 | 61.0 | 60.4 |
| Outflow Channel Landforms in Promethei Terra : ESP_049804_1425 ESP_057360_1425 (Interval in Earth days: 588) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.0 | 102. | 4.46 | 21.38 | 38.3 | 34.6 |
| USGS Dune Database Entry Number 1541-381 : ESP_049723_1415 ESP_050224_1415 (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 | -38.2 | 154. | 3.30 | 22.10 | 38.0 | 44.0 |
| Summit of Argyre Mons : ESP_050047_1295 ESP_050271_1295 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -50.3 | 312. | -5.0 | 24.23 | 51.5 | 53.6 |
| Faults and Pitted Mounds in Utopia Planitia : ESP_050094_2150 ESP_050305_2150 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.46 | 96.0 | 5.52 | -6.61 | 49.3 | 47.5 |
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