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.
| Group of Cones with Summit Depressions near Coprates Chasma North Wall: ESP_036109_1675 ESP_043520_1675 (Interval in Earth days: 577) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.4 | 297. | 0.39 | 26.06 | 62.1 | 55.2 |
| Summit Pit Crater in Terra Sirenum: ESP_036086_1470 ESP_036574_1470 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -32.9 | 207. | 6.31 | -16.4 | 75.2 | 74.5 |
| East Rim of Well-Preserved Impact Crater: ESP_036335_2270 ESP_036757_2270 (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 | 46.55 | 239. | 6.41 | -5.27 | 46.7 | 51.9 |
| Chasma Boreale Gypsum Dune Changes: ESP_036118_2650 ESP_027495_2650 (Interval in Earth days: 672) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 84.97 | -1.9 | 8.93 | -5.29 | 62.2 | 64.2 |
| Crater in Central Arabia Terra with Yardangs at Northeast Wall: ESP_036290_1915 ESP_037358_1915 (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 | 11.36 | 33.7 | -4.3 | 14.11 | 50.7 | 53.3 |
| Small Rocky Impact Crater: ESP_036303_1680 ESP_037160_1680 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.7 | 42.0 | -8.9 | 14.53 | 62.0 | 58.5 |
| Vastitas Borealis Intra-Crater Dunes: ESP_036344_2520 ESP_036463_2520 (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 | 71.89 | 344. | 8.11 | -18.5 | 56.2 | 59.4 |
| Crater Near Center of Sinai Planum: ESP_036255_1665 ESP_053793_1665 (Interval in Earth days: 1367) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.3 | 271. | 6.61 | -5.08 | 62.1 | 60.2 |
| Topographic Low with Thermally-Distinct Terrain in THEMIS IR Images: ESP_036135_2185 ESP_036979_2185 (Interval in Earth days: 65) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.54 | 301. | 0.45 | -20.5 | 44.9 | 54.1 |
| InSight Mission Candidate Landing Site: ESP_036273_1840 ESP_036207_1840 (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 | 4.093 | 137. | 5.69 | 24.35 | 52.8 | 51.3 |
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