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.
| Ridges Radial To Wall of Crater: ESP_027072_1620 ESP_035221_1620 (Interval in Earth days: 635) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -17.9 | 59.5 | -6.6 | 11.48 | 64.9 | 64.2 |
| One Kilometer Diameter Crater on Northern Plains: ESP_027073_2410 ESP_027851_2410 (Interval in Earth days: 60) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 60.47 | 20.7 | -3.4 | 8.207 | 47.8 | 53.6 |
| Candidate Future Landing Site in Schiaparelli Crater: ESP_027311_1755 ESP_028432_1755 (Interval in Earth days: 87) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.25 | 13.3 | -6.9 | -17.7 | 56.3 | 56.3 |
| Ius Chasma Dune Changes: ESP_027341_1720 ESP_027064_1720 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.71 | 276. | -24. | -4.20 | 59.5 | 58.2 |
| Potential Landing Site in Mawrth Vallis: ESP_027378_2060 ESP_027655_2060 (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 | 25.46 | 339. | 6.81 | -8.49 | 44.0 | 46.7 |
| 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 |
| Flows and Terraces Overlapping Crater Ejecta South of Marte Vallis: ESP_027318_1860 ESP_027595_1860 (Interval in Earth days: 21) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 5.876 | 180. | -5.0 | -22.2 | 51.0 | 52.7 |
| Circular Feature in Tharsis Region: ESP_027197_1975 ESP_026353_1975 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.35 | 242. | -5.6 | 7.809 | 46.4 | 43.2 |
| 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 |
| 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 |
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