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 Material in Melas Chasma: PSP_002630_1695 PSP_005953_1695 (Interval in Earth days: 259) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -10.2 | 286. | 7.88 | -11.5 | 55.6 | 34.6 |
Pit Craters of Tractus Catena: PSP_002420_2040 PSP_002710_2040 (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 | 23.82 | 256. | -2.8 | 23.57 | 57.1 | 57.8 |
Mantled Surface of Ascraeus Mons: PSP_002196_1920 PSP_002618_1920 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.66 | 252. | 4.69 | -8.52 | 53.6 | 57.1 |
Tongue-Shaped Flow Feature in Hellas Planitia: PSP_002320_1415 PSP_003243_1415 (Interval in Earth days: 72) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -38.1 | 113. | 8.81 | 20.07 | 66.6 | 53.8 |
Portion of Beagle 2 Landing Ellipse in Isidis Planitia: PSP_002347_1915 ESP_015968_1915 (Interval in Earth days: 1061) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 11.58 | 90.7 | -3.0 | -28.4 | 55.1 | 41.8 |
Northern Hemisphere Gullies with Layers: PSP_001528_2210 PSP_002214_2210 (Interval in Earth days: 53) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 40.58 | 120. | 2.07 | -20.9 | 49.9 | 60.6 |
Unusual Structure on Crater Rim in West Utopia Planitia: PSP_001503_2180 PSP_001978_2180 (Interval in Earth days: 37) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.53 | 82.7 | 0 | -14.8 | 49.4 | 56.0 |
Slope Streaks in Acheron Fossae: PSP_001656_2175 PSP_002632_2175 (Interval in Earth days: 76) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.31 | 229. | 0.77 | -25.4 | 50.8 | 65.6 |
Oudemans Crater Central Uplift: A Sample of Well-Preserved Layering: PSP_001602_1700 PSP_002446_1700 (Interval in Earth days: 66) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -9.91 | 268. | 2.60 | 26.00 | 58.6 | 54.6 |
Evidence of Multiple Episodes of Gully Formation: PSP_001684_1410 PSP_002027_1410 (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 | -38.8 | 196. | -6.7 | -25.8 | 74.3 | 72.5 |
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