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.
| Sublimation Process and Spider Evolution : PSP_002758_0945 PSP_002759_0855 (Interval in Earth days: 0) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -85.4 | 104. | -20. | -25.0 | 87.6 | 89.1 |
| Layered Deposits within an Unnamed Crater in Arabia Terra: PSP_002100_1840 ESP_060054_1840 (Interval in Earth days: 4515) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.165 | 354. | 0 | -10.2 | 54.3 | 38.9 |
| Incipient Gullies, As Seen in MOC Image M20-00901: PSP_002146_1335 PSP_002423_1335 (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 | -46.1 | 184. | 6.03 | -15.6 | 73.1 | 71.0 |
| Crater and Extensive Field of Secondary Craters Seen in MOC Image R15-02146: PSP_002230_1850 ESP_027890_1850 (Interval in Earth days: 1999) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.727 | 46.1 | -7.8 | 4.118 | 55.2 | 51.4 |
| Blocks in the Olympus Mons : PSP_003450_1975 ESP_012060_1975 (Interval in Earth days: 671) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.42 | 216. | 2.71 | 26.11 | 61.9 | 60.8 |
| Sand Dunes in Rabe Crater: PSP_002824_1355 PSP_003325_1355 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -43.9 | 34.5 | 4.86 | 26.51 | 63.0 | 53.6 |
| Possible Cinder Cone on the Southern Flank of Pavonis Mons: PSP_002671_1790 ESP_011413_1790 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.10 | 246. | -2.3 | -18.2 | 55.8 | 58.8 |
| Candidate Cavern Entrance Northeast of Arsia Mons: PSP_003647_1745 PSP_004847_1745 (Interval in Earth days: 94) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -5.53 | 241. | -0.5 | -16.3 | 52.3 | 41.1 |
| Very Fine Layers in Juventae Chasma: PSP_002590_1765 PSP_002946_1765 (Interval in Earth days: 28) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.29 | 298. | -2.1 | 6.197 | 55.9 | 54.9 |
| Ares Vallis Cataract: PSP_003538_1885 PSP_004171_1885 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.380 | 335. | -1.1 | -19.6 | 58.1 | 56.2 |
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