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.
| Mounds in Cydonia Region: PSP_007770_2205 PSP_007981_2205 (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 | 40.03 | 345. | 7.20 | -6.26 | 41.7 | 42.5 |
| Faulted Layered Deposits in Eastern Candor Chasma: PSP_007192_1710 PSP_008049_1710 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.72 | 295. | 7.77 | -11.1 | 45.4 | 55.7 |
| Northwest Hellas Basin Landforms: PSP_007636_1400 ESP_016075_1400 (Interval in Earth days: 658) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.4 | 55.9 | 0.23 | -23.1 | 71.3 | 67.4 |
| Light-Toned Outcrops in North Melas Chasma Wall with Possible Sulfates: PSP_007390_1700 PSP_007680_1700 (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 | -9.78 | 289. | -8.0 | 6.442 | 49.4 | 51.7 |
| Landslide Scarp: PSP_007785_1645 PSP_008141_1645 (Interval in Earth days: 27) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.1 | 303. | 7.47 | -3.79 | 56.0 | 60.0 |
| Gullies as Seen in MOC Image M02-02681: PSP_007213_1400 ESP_042618_1400 (Interval in Earth days: 2759) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -39.6 | 86.3 | 2.71 | 26.46 | 65.4 | 65.6 |
| Deposits in Kasei Valles: PSP_007970_2015 ESP_033551_2015 (Interval in Earth days: 1993) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.06 | 287. | -0.6 | 17.86 | 42.0 | 36.8 |
| Possible Sulfates in Coprates Chasma: PSP_007205_1660 ESP_024505_1660 (Interval in Earth days: 1348) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -13.9 | 301. | 5.58 | -16.3 | 48.4 | 44.1 |
| Central Peak of Large Crater in Northwest Arabia Terra: PSP_007664_2160 ESP_045443_2160 (Interval in Earth days: 2944) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 35.80 | 0.55 | 8.68 | -7.28 | 40.8 | 44.8 |
| Middle Section of Northern Olympus Mons Basal Scarp: PSP_007089_2035 PSP_007946_2035 (Interval in Earth days: 67) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.25 | 223. | 7.43 | -6.64 | 38.8 | 42.1 |
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