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.
| Pedestal Crater Near Phoenix Landing Site: ESP_062089_2485 ESP_061891_2485 (Interval in Earth days: 15) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 68.23 | 233. | -13. | 5.964 | 51.1 | 49.2 |
| Clay-Bearing Landslide and Outcrop in Degraded Crater: ESP_061990_1770 ESP_062056_1770 (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 | -2.77 | 65.1 | 5.98 | -13.8 | 54.3 | 55.8 |
| Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater: ESP_061950_1990 ESP_062095_1990 (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 | 18.67 | 77.4 | -27. | -11.1 | 46.6 | 45.5 |
| Flow Margin in Phlegra Dorsa: ESP_061854_2080 ESP_061920_2080 (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 | 27.85 | 173. | 8.37 | -7.74 | 40.8 | 42.4 |
| Arcuate Fractures in Utopia Planitia: ESP_062081_2125 ESP_061936_2125 (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 | 32.00 | 95.9 | 8.81 | -8.52 | 40.8 | 41.9 |
| Flow Deposits in Eastern Ladon Valles: ESP_062099_1620 ESP_062534_1620 (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 | -17.9 | 332. | -6.1 | 19.86 | 65.0 | 63.4 |
| Crater in Arabia Terra: ESP_062071_2185 ESP_061926_2185 (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 | 38.36 | 7.97 | 9.64 | -6.81 | 40.5 | 41.5 |
| Ice-Filled Crater in North Polar Layered Deposits: ESP_062085_2645 ESP_062203_2645 (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 | 84.40 | 315. | 0.89 | 14.85 | 59.7 | 59.7 |
| Crater in Arabia Terra: ESP_061992_2120 ESP_062915_2120 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.49 | 5.72 | 8.74 | -10.3 | 40.7 | 47.3 |
| Coprates Chasma Dune Changes: ESP_062153_1660 ESP_062219_1660 (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 | -13.9 | 296. | -1.0 | -25.8 | 62.1 | 63.9 |
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