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 Noctis Region: ESP_017979_1715 ESP_018401_1715 (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 | -8.26 | 267. | -7.1 | -21.7 | 59.6 | 60.6 |
Crater Floor Depressions: ESP_017934_2025 ESP_018435_2025 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 22.32 | 53.1 | -13. | 7.638 | 45.4 | 44.9 |
Nozzle for Scarp-Fed Sands: ESP_017871_2745 ESP_026613_2745 (Interval in Earth days: 681) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 85.24 | 183. | 2.61 | -7.04 | 65.2 | 66.3 |
Impact Crater in Northern Plains: ESP_018037_2445 ESP_018828_2445 (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 | 64.01 | 110. | 7.02 | 25.87 | 48.1 | 51.9 |
Exposures of Various North Polar Geologic Units: ESP_017845_2625 ESP_018016_2625 (Interval in Earth days: 13) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 82.42 | 302. | -5.5 | 9.318 | 58.6 | 58.2 |
Amazonis Planitia: ESP_017836_1970 ESP_017981_1970 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 16.64 | 209. | -11. | 2.253 | 46.8 | 46.0 |
Exposure of Polar Layered Deposits: ESP_018096_2710 ESP_018071_2690 (Interval in Earth days: 2) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 88.99 | 190. | -17. | -17.5 | 64.8 | 64.3 |
Pits and Craters: ESP_017875_2305 ESP_018007_2305 (Interval in Earth days: 10) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 49.95 | 219. | -4.6 | -28.8 | 43.8 | 46.5 |
Northern Wall of Kasei Valles: ESP_017859_2120 ESP_018492_2120 (Interval in Earth days: 49) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 31.52 | 297. | 10.8 | -7.29 | 41.3 | 45.0 |
Disrupted Blocky Outcrop in Cerberus Palus: ESP_018036_1880 ESP_043710_1880 (Interval in Earth days: 2001) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 8.089 | 149. | -6.4 | 6.703 | 50.5 | 45.5 |
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