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.
| Two Circular Cracked Surfaces in Northeast Acidalia Planitia: ESP_027035_2265 ESP_045958_2265 (Interval in Earth days: 1474) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.21 | 340. | 2.61 | -25.0 | 42.8 | 55.2 |
| Modified Crater on Northern Plains: ESP_027027_2325 ESP_027370_2325 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 52.35 | 197. | 4.31 | -17.9 | 44.0 | 48.1 |
| Candidate Future Landing Site North of Echus Chaos: ESP_027090_1955 ESP_026602_1955 (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 | 15.09 | 284. | -14. | 11.82 | 47.6 | 44.5 |
| Layers around Mound in Protonilus Mensae: ESP_027072_2275 ESP_027850_2275 (Interval in Earth days: 61) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 47.37 | 50.1 | 0 | 16.21 | 43.4 | 48.1 |
| Chasma Boreale Linear Dune Changes: ESP_027075_2630 ESP_027114_2630 (Interval in Earth days: 3) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 83.14 | 314. | -9.2 | 8.368 | 60.3 | 59.6 |
| Overlapping Pedestal Craters in THEMIS Image V20104004: ESP_027334_2345 ESP_027954_2345 (Interval in Earth days: 48) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 54.00 | 95.4 | 7.10 | -20.0 | 46.1 | 54.6 |
| Valley Features Among Ridges in Arsia Sulci Region: ESP_027303_1765 ESP_028635_1765 (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 | -3.32 | 230. | 1.40 | -12.3 | 55.3 | 55.6 |
| Light Outcrops in Iani Chaos: ESP_027022_1785 ESP_079309_1785 (Interval in Earth days: 4074) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.58 | 341. | 0 | 18.78 | 54.3 | 55.3 |
| Chaos and Outflow Channel Floor Transition in Osuga Valles: ESP_027392_1650 ESP_027880_1650 (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 | -15.0 | 322. | 8.60 | -5.08 | 61.6 | 61.1 |
| Central Peak of Fournier Crater in Tyrrhena Terra: ESP_027322_1755 ESP_027810_1755 (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 | -4.38 | 72.6 | -1.4 | -16.4 | 56.0 | 56.7 |
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