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.
| 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 |
| Unnamed Small Rayed Crater in Hesperia Region: PSP_008135_1520 PSP_008425_1520 (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 | -27.9 | 108. | -4.0 | 6.037 | 68.6 | 70.2 |
| 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 |
| Slope Streaks Beginning at Stratigraphic Layers: PSP_007473_1850 PSP_008264_1850 (Interval in Earth days: 62) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 4.996 | 181. | -5.4 | 5.46 | 43.6 | 48.7 |
| Stair-Stepped Slope Seen in MOC Image R08-00823: PSP_007684_1795 ESP_020171_1795 (Interval in Earth days: 973) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -0.44 | 180. | -5.7 | 17.22 | 47.7 | 53.5 |
| Wrinkle Ridge in Hesperia Planum: PSP_007726_1560 PSP_008082_1560 (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 | -23.9 | 115. | 8.10 | -3.05 | 61.0 | 65.3 |
| 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 |
| Mangala Valles: PSP_008118_1645 PSP_008408_1645 (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 | -15.5 | 210. | 4.85 | 15.67 | 59.6 | 61.0 |
| Wall Layers of Tooting Crater: PSP_007907_2035 ESP_019115_2035 (Interval in Earth days: 873) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 23.18 | 208. | -2.3 | 5.434 | 41.6 | 48.0 |
| Light-Toned Layered Deposits Along Plains South of Ius Chasma: PSP_007786_1710 PSP_009935_1710 (Interval in Earth days: 167) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.74 | 276. | -4.8 | 20.55 | 52.9 | 58.8 |
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