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.
| Gullied Slope: ESP_064885_1405 ESP_065518_1405 (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 | -39.3 | 229. | -7.2 | 6.96 | 59.0 | 49.3 |
| Icaria Planum: ESP_064832_1405 ESP_074012_1400 (Interval in Earth days: 715) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.3 | 235. | 2.82 | -7.26 | 59.0 | 54.2 |
| Valleys in Crater Northeast of Argyre Planitia: ESP_064736_1500 ESP_064591_1500 (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 | -29.7 | 335. | 0.30 | -16.8 | 58.2 | 61.0 |
| Candidate ExoMars Landing Site in Oxia Planum: ESP_064828_1985 ESP_064538_1985 (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 | 18.21 | 335. | 20.9 | -12.9 | 61.2 | 61.8 |
| Sublimation at Spiders Site: ESP_064785_0930 ESP_064639_0930 (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 | -87.0 | 127. | 8.53 | 21.89 | 80.1 | 81.5 |
| Layering in Arabia Terra: ESP_064616_1820 ESP_064761_1820 (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 | 2.180 | 6.47 | 6.15 | 23.87 | 57.5 | 56.2 |
| Mounds in Oxia Colles: ESP_064604_1985 ESP_064459_1985 (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 | 18.44 | 331. | 8.61 | -7.88 | 60.7 | 60.8 |
| Channel: ESP_064748_1765 ESP_065724_1765 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.41 | 3.86 | 3.24 | -8.49 | 57.1 | 53.8 |
| Aprons with Channels in Eos Chasma: ESP_064697_1665 ESP_064842_1665 (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 | -13.3 | 317. | 0.00 | 19.25 | 56.9 | 54.7 |
| Miyamoto Crater: ESP_064788_1765 ESP_064854_1765 (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 | -3.30 | 352. | 1.63 | -19.2 | 57.2 | 58.8 |
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