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.
Possible Submarine Fan in Eastern Portion of Small Melas Chasma Basin: PSP_007377_1700 PSP_008379_1700 (Interval in Earth days: 78) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.82 | 283. | 5.56 | -6.99 | 48.4 | 58.5 |
Granicus Valles Subchannel Breakout From Main Channel: PSP_007725_2075 PSP_007936_2075 (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 | 27.11 | 136. | 7.86 | -8.35 | 40.0 | 41.8 |
Complex Layered Deposits in Tithonium Chasma: PSP_007918_1755 PSP_008274_1755 (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 | -4.64 | 270. | 6.16 | -5.59 | 51.1 | 54.6 |
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 |
Dune Field in Impact Crater Near Cerberus Fossae: PSP_008159_1885 PSP_008449_1885 (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 | 8.564 | 169. | -6.9 | 2.406 | 47.4 | 48.2 |
Layering in East Coprates Chasma Wall: PSP_007864_1655 PSP_007508_1655 (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 | -14.1 | 307. | -8.1 | 4.599 | 57.2 | 52.4 |
Light-Toned Tilted Layering in Central Peak of Oudemans Crater: PSP_007694_1700 ESP_027882_1700 (Interval in Earth days: 1574) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.92 | 268. | 1.09 | -17.4 | 52.3 | 59.3 |
Polygonal Fractures in Utopia Planitia: PSP_008069_2195 PSP_008504_2195 (Interval in Earth days: 34) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.95 | 102. | -5.9 | 5.466 | 42.2 | 41.3 |
Ganges Mensa: PSP_007521_1725 PSP_007877_1725 (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 | -7.23 | 311. | 7.88 | -4.81 | 48.5 | 53.0 |
Light-Toned Outcrops Exhumed From Dark Material in Arabia Terra: PSP_008139_1905 PSP_009576_1905 (Interval in Earth days: 112) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 10.54 | 355. | -7.9 | 17.40 | 46.6 | 49.4 |
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