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.
| Ridges and Mounds Near Hecates Tholus: PSP_007672_2155 PSP_007883_2155 (Interval in Earth days: 16) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.92 | 142. | 6.64 | -7.98 | 40.8 | 42.0 |
| Valley Juncture Along Plains West of Ganges Chasma with Light-Toned Deposit: PSP_008009_1715 PSP_009578_1715 (Interval in Earth days: 122) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.51 | 306. | 1.52 | -24.6 | 54.4 | 62.1 |
| Alluvial Fan Apex in Saheki Crater: PSP_007543_1580 PSP_007899_1580 (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 | -21.7 | 72.5 | 3.97 | -8.11 | 57.6 | 62.4 |
| Dark Dune-Like Forms in Southern Melas Chasma: PSP_007522_1685 ESP_025666_1685 (Interval in Earth days: 1414) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -11.1 | 284. | 0.94 | -27.7 | 51.1 | 56.6 |
| Wrinkle Ridge: PSP_007052_1870 ESP_016361_1870 (Interval in Earth days: 726) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 7.101 | 156. | -6.0 | 26.66 | 39.8 | 40.6 |
| Putative Salt Deposits Detected by THEMIS West of Meridiani Region: PSP_007981_1770 PSP_008851_1770 (Interval in Earth days: 68) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -3.06 | 350. | -5.6 | 23.21 | 51.6 | 54.5 |
| Rayed Crater with Central Peak at Acidalia Planitia-Arabia Terra Boundary: PSP_007123_2250 ESP_023803_2250 (Interval in Earth days: 1300) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 44.71 | 12.7 | -0.0 | 26.95 | 46.9 | 54.3 |
| Rocky Central Uplift of 80-Kilometer Diameter Crater: PSP_007978_2005 ESP_024487_2005 (Interval in Earth days: 1286) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 20.18 | 69.4 | 0 | -26.2 | 42.1 | 39.4 |
| Cut Crater in Ganges Chasma: PSP_008101_1710 ESP_016263_1710 (Interval in Earth days: 636) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -8.91 | 314. | -5.3 | 21.95 | 55.9 | 47.3 |
| Possible Sulfates in Ius Chasma: PSP_007509_1720 ESP_050839_1720 (Interval in Earth days: 3376) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.70 | 279. | -2.3 | 13.43 | 49.3 | 36.5 |
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