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.
| 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 |
| 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 |
| Alba Mons Northwest Caldera Wall: ESP_077730_2210 ESP_077809_2210 (Interval in Earth days: 6) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.78 | 249. | -5.4 | 18.85 | 46.3 | 44.0 |
| Crater in Arabia Terra: ESP_077607_2180 ESP_078029_2180 (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 | 37.81 | 5.52 | 19.9 | -4.06 | 43.7 | 44.1 |
| Ridge in Claritas Fossae: ESP_077506_1515 ESP_077031_1515 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -28.3 | 254. | -5.4 | 20.01 | 55.9 | 46.9 |
| Possible Phyllosilicates Associated with Small Crater in Tyrrhena Terra: ESP_077657_1665 ESP_076760_1665 (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 | -13.3 | 89.1 | 0.02 | 14.13 | 49.1 | 37.1 |
| Traverse Ramp in East Coprates Chasma: ESP_077504_1640 ESP_076396_1640 (Interval in Earth days: 86) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.8 | 306. | 1.04 | -18.0 | 48.3 | 37.1 |
| Eastern Ejecta and Rays of Gasa Crater: ESP_077537_1440 ESP_077471_1440 (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 | -35.6 | 129. | -8.7 | 5.462 | 61.4 | 59.5 |
| Looking at the Crater Half Full: ESP_076968_1475 ESP_076823_1475 (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 | -32.4 | 173. | 23.4 | -6.17 | 48.0 | 47.6 |
| Layers in West Melas Chasma: ESP_077109_1715 ESP_077043_1715 (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 | -8.53 | 285. | -7.5 | 6.737 | 41.0 | 39.2 |
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