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.
| Athabasca Valles Side Channel: ESP_077905_1880 ESP_079329_1880 (Interval in Earth days: 111) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.854 | 154. | -2.7 | 15.05 | 43.5 | 50.5 |
| Ridge Network in Hellas Planitia: ESP_077843_1420 ESP_086717_1420 (Interval in Earth days: 692) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -37.6 | 53.8 | -2.3 | 22.29 | 67.0 | 66.0 |
| Ascraeus Mons Southern Caldera Wall: ESP_078165_1910 ESP_078455_1910 (Interval in Earth days: 23) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.88 | 255. | -2.7 | 22.24 | 44.5 | 44.5 |
| Traverse Ramp in East Coprates Chasma: ESP_077926_1640 ESP_078361_1640 (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 | -15.6 | 306. | -27. | 4.196 | 55.8 | 58.5 |
| Exposed Stratigraphy in Peraea Cavus Southern Wall: ESP_077960_1500 ESP_078171_1500 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -29.7 | 95.5 | 24.1 | 12.30 | 61.6 | 65.1 |
| Northern Mid-Latitude Terrain: ESP_078015_2195 ESP_086309_2195 (Interval in Earth days: 646) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.43 | 26.7 | 3.22 | -6.74 | 44.0 | 46.9 |
| Climbing Dunes Escaping a Crater in Aonia Terra: ESP_039380_1290 ESP_039657_1290 (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 | -50.4 | 293. | 6.25 | -11.6 | 46.2 | 44.6 |
| Channels Intersecting Crater in Xanthe Terra: ESP_077702_1755 ESP_076805_1755 (Interval in Earth days: 70) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -4.60 | 301. | -27. | -7.96 | 47.8 | 37.6 |
| Dune Changes near Martz Crater: ESP_077629_1420 ESP_077919_1420 (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 | -37.7 | 136. | 4.84 | 19.09 | 63.4 | 66.9 |
| Monitor Gullies and Lobes in Can Crater : ESP_077555_2285 ESP_077344_2285 (Interval in Earth days: 17) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 48.21 | 345. | 4.73 | -6.81 | 50.4 | 53.1 |
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