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.
Central Peak and South Rim of Large Fresh Crater in Isidis Basin: PSP_007107_1900 PSP_009823_1900 (Interval in Earth days: 211) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.02 | 94.3 | 0.07 | -12.8 | 39.2 | 52.4 |
Floor and Central Uplift of Mazamba Crater in Thaumasia Planum: PSP_007100_1520 ESP_033248_1520 (Interval in Earth days: 2038) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -27.5 | 290. | -1.6 | -23.6 | 55.6 | 51.8 |
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 |
Region Showing Differentially-Eroded Distal Fan Deposits: PSP_007688_1575 PSP_008545_1575 (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 | -22.0 | 72.9 | 6.99 | -15.6 | 59.4 | 68.1 |
Hellas Planitia: PSP_007781_1410 PSP_008137_1410 (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 | -38.4 | 55.7 | 6.07 | -3.19 | 72.0 | 76.2 |
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 |
Central Peak of Fesenkov Crater: PSP_007931_2020 ESP_024585_2020 (Interval in Earth days: 1298) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.68 | 273. | -8.3 | -25.5 | 42.4 | 39.6 |
Central Peak Region of Canso Crater: PSP_007139_2015 ESP_085442_2015 (Interval in Earth days: 6101) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 21.34 | 299. | -1.5 | -10.2 | 39.3 | 44.2 |
Interaction between Unnamed Crater Ejecta and Pre-Exsisting Terrain: PSP_007681_2000 PSP_008406_2000 (Interval in Earth days: 57) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 19.66 | 259. | -6.6 | 23.65 | 41.5 | 41.9 |
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