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.
| Hillslope Morphologies near Murray Crater: ESP_087074_1555 ESP_087219_1555 (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 | -24.0 | 28.1 | -7.1 | 10.08 | 63.0 | 63.5 |
| North-Pole-Facing Deposit in Crater Associated with Headwall Erosion: ESP_087078_2245 ESP_087144_2245 (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 | 44.13 | 268. | 3.97 | -10.9 | 44.1 | 45.1 |
| Southern Canyon Wall in East Coprates Chasma: ESP_087077_1640 ESP_079350_1640 (Interval in Earth days: 602) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.6 | 304. | -0.9 | 15.12 | 57.2 | 64.5 |
| Channeled Terraces and Debris Fan in Crater in Arabia Terra: ESP_087022_2165 ESP_087167_2165 (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 | 35.93 | 0.65 | -9.7 | 3.05 | 43.4 | 42.1 |
| Layering in Lucus Planum: ESP_087187_1715 ESP_087464_1715 (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 | -8.22 | 177. | 29.2 | 6.933 | 51.7 | 55.7 |
| Volcanic Vent Southeast of Pavonis Mons: ESP_086802_1790 ESP_087079_1790 (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 | -1.03 | 249. | 8.99 | -22.0 | 45.9 | 50.7 |
| Pitted Cone with Clear Moat: ESP_086926_2080 ESP_087071_2080 (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 | 27.85 | 102. | -8.9 | 4.814 | 42.3 | 41.3 |
| Crater Wall with Potential Chloride Deposit Outcrop: ESP_086817_1465 ESP_090153_1465 (Interval in Earth days: 260) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -33.3 | 205. | -2.0 | 16.07 | 65.8 | 68.4 |
| Concentric Crater Fill: ESP_087124_2205 ESP_087190_2205 (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 | 40.20 | 93.4 | 5.73 | -9.98 | 42.7 | 43.9 |
| High-Latitude Crater: ESP_086952_2425 ESP_088099_2425 (Interval in Earth days: 90) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 62.05 | 104. | 3.58 | 29.37 | 52.9 | 45.4 |
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