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.
| Well-Preserved Impact Crater : ESP_028830_2040 ESP_042043_2040 (Interval in Earth days: 1030) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.59 | 303. | -5.3 | -28.5 | 55.9 | 42.2 |
| Layering in Crater in Mawrth Vallis : ESP_028855_2045 ESP_020297_2045 (Interval in Earth days: 666) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.23 | 341. | -13. | -25.2 | 57.0 | 61.1 |
| Arsia Mons Southern Caldera Wall Upper Flank and Caldera Floor : ESP_028872_1695 ESP_082280_1695 (Interval in Earth days: 4161) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.1 | 239. | 6.91 | -4.71 | 55.2 | 58.1 |
| Olympica Fossae : ESP_028898_2050 ESP_036691_2050 (Interval in Earth days: 607) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 24.72 | 245. | 5.26 | -17.8 | 56.0 | 50.5 |
| Flow Boundary in Tharsis Region East of Pavonis Mons : ESP_028621_1775 ESP_034291_1775 (Interval in Earth days: 442) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -2.48 | 251. | 3.73 | -19.1 | 54.2 | 50.4 |
| Distorted Icy Terrain in Nilosyrtis Mensae Crater : ESP_028601_2145 ESP_028324_2145 (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 | 34.17 | 73.6 | -1.8 | 13.89 | 55.3 | 50.7 |
| Possible Repetitive Bedding Near Base of Central Lobe of Medusae Fossae : ESP_028650_1695 ESP_028795_1695 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.4 | 180. | 8.61 | 21.62 | 55.7 | 54.2 |
| Northeast Melas Chasma Dune Fields and Wall Rock : ESP_028857_1700 ESP_028923_1700 (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 | -10.0 | 290. | -4.8 | -26.4 | 56.1 | 57.7 |
| Pavonis Mons Reticulate Bedform Change Detection : ESP_028608_1805 ESP_028542_1805 (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 | 0.517 | 247. | -6.2 | 18.32 | 54.3 | 52.4 |
| Olympus Mons Aureole Ripple Change Detection : ESP_028754_1975 ESP_028820_1975 (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 | 17.06 | 217. | 6.54 | -15.4 | 53.3 | 55.6 |
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